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36.Commission De La Theorie Des Atmospheres Stellaires

Published online by Cambridge University Press:  25 April 2016

Abstract

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Reports of Commissions
Copyright
Copyright © Reidel 1967

References

Bibliography

I. Books, Proceedings of Colloquia and Symposia

1. Proc. First Harvard-Smithsonian Conference on Stellar Atmospheres (Model Stellar Atmospheres), Cambridge (Mass.) 1964.Google Scholar
2. Proc. Second Harvard-Smithsonian Conference on Stellar Atmospheres: The Formation of Spectrum Lines, ed. Avrett, E. H., Gingerich, O., Whitney, C. A., Cambridge (Mass.) 1965.Google Scholar
3. Proc. IAU Colloquium: The Blanketing Effect, ed. Böhm, K.-H, J. quantit. Spectrosc. radiat. Transfer, 6, no. 5, 1966.Google Scholar
4. Thomas, R. N. 1965, Non-Equilibrium Thermodynamics in the Presence of a Radiation Field, University of Colorado Press.Google Scholar
5. The Solar Spectrum, ed. de Jager, C.. D. Reidel Publ. Co., Dordrecht-Holland, 1965.Google Scholar
6. Proc. IAU Symposium no. 26: Abundance Determinations in Stellar Spectra, ed. Hubenet, H., Academic Press, 1966.Google Scholar
7. Sobolev, V. V., Gorbatzky, V. G., Ivanov, V. V. (ed.) 1966, Theory of Stellar Spectra, ‘Nauka’ Publ. Co., Moscow.Google Scholar
8. Sampson, D. H. 1965, Radiative Contributions to Energy and Momentum Transport in a Gas, Interscience Publ.Google Scholar
9. Underhill, A. B. 1966, The Early-Type Stars, Reidel Publ. Co., Dordrecht.CrossRefGoogle Scholar
10. Proc. IAU Symposium No. 22: Stellar and Solar Magnetic Fields, ed. Lüst, R., North Holland Pub. Co., Amsterdam, 1965.Google Scholar
11. Review articles: Pecker, J.-C. Model Atmospheres, in A. Rev. Astr. Astrophys, 3, 135.CrossRefGoogle Scholar
Regemorter, H. van Spectral Line Broadening, A. Rev. Astr. Astrophys., 3, 71.CrossRefGoogle Scholar
Cayrel, R., Cayrel, G. 1966, Abundance Determination from Stellar Spectra, A. Rev. Astr. Astrophys., 4, 1.CrossRefGoogle Scholar
1. Sampson, D. H. 1965, Radiative Contributions to Energy and Momentum Transport in a Gas. Interscience Publishers.Google Scholar
2. Cayrel, R. 1966, The Line Blanketing Problem in the Non-LTE Approach. J. quantit, Spectrosc, radiat. Transfer, 6, 621.CrossRefGoogle Scholar
3. Kalkofen, W., Avrett, H. 1965, Solution of the Line and Continuum Transfer Problem for a 3-Level Atom. Proc. 2nd Harvard-Smiths. Conf. on Stellar Atmospheres, p, 249.Google Scholar
4. Ambarzumian, V. A. 1964, On a Non-Linear Problem of Light Scattering in a Turbid Medium. Dokl. Akad. Nauk Armjam. SSR, 38, 225.Google Scholar
5. Ambarzumian, V. A. 1964, On one Case of Diminishing of Optical Thickness of a Medium under the Action of Radiation. Dokl. Akad. Nauk Armjan. SSR, 39, 159.Google Scholar
6. Johnson, H. R., Klinglesmith, D. A. 1965, Proc. 2nd Harvard- Smithson, Conf. on Stellar Atmospheres, 221.Google Scholar
7. Bellman, R., Kalaba, R., Ueno, S. 1964, Invariant Imbedding and Time-Dependent Scattering of Light in a One-Dimensional Medium. J. Math. Analysis and Applications, 9, 424.CrossRefGoogle Scholar
8. Bellman, R., Kalaba, R., Ueno, S. 1964, Invariant Imbedding and Scattering of Light in a One-Dimensional Medium with a Moving Boundary. The Rand Corp., Mem. RM-3960-ARPA.CrossRefGoogle Scholar
9. Bellman, R., Kalaba, R., Ueno, S. 1964, Invariant Imbedding and a Resolvent of the Photon-Diffusion Equation. The Rand Corp., Mem. RM-3937-ARPA.Google Scholar
10. Bellman, R., Kalaba, R., Kagiwada, H., Ueno, S. The Invariant Imbedding Equation for the Dissipation Function of a Homogeneous Finite Slab, The Rand Corp., Mem. RM-4651-NASA. Q. J. Appl. Math, (in press).Google Scholar
11. Bellman, R., Kagiwada, H., Kalaba, R. 1966, Invariant Imbedding and a Reformulation of the Internal Intensity Problem in Radiative Transfer. Mon. Not. R. astr. Soc., 132, 183.CrossRefGoogle Scholar
12. Bellman, R., Kagiwada, H., Kalaba, R. 1966, Numerical Results for the Auxiliary Equation of Radiative Transfer, J. quantit. Spectrosc. rad. Transfer, 6, 291.CrossRefGoogle Scholar
13. Bellman, R., Kagiwada, H., Kalaba, R., Ueno, S. 1966, Numerical Results for Chand- rasekhar's X- and Y-Functions of Radiative Transfer. J. quantit. Spectrosc. rad. Transfer. 6, 479.CrossRefGoogle Scholar
14. Biberman, L. M., Vorobyev, V. S., Lagar'kov, A. N. 1965, Transfer of Radiation in an Ionization Continuum. Optica i Spectroscopia, 19, 326.Google Scholar
15. Böhm, K.-H. 1965, Temperaturinversion in einer Atmosphare im nichtgrauen Strahlungsgleichgewicht. Z. Astrophys,, 62, 167.Google Scholar
16. Böhm, K.-H., Deinzer, W. 1965, Atmosphären von Zentralsternen planetarischer Nebel, I. Z. Astrophys., 61, 1.Google Scholar
17. Carlstedt, J. L., Mullikin, T. W. 1966, Chandrasekhar's X- and Y-Functions. Astrophys, J., 12, 449.CrossRefGoogle Scholar
18. Chapman, R. J. 1966, Radiative Transfer in Extended Stellar Atmospheres. Astrophys. J., 143, 61.CrossRefGoogle Scholar
19. Collins, G. W. II, Code, A. D. 1965, Some Numerical Methods for the Solution of the Equation of Transfer. Astrophys. J., 142, 1576.CrossRefGoogle Scholar
20. Cuny, Y. 1964, Solution of the Transfer Problem. Proc. Second Harvard Smithson. Conf. C. r. Acad. Sci. Paris, 258, 3292.Google Scholar
21. Dave, J. V., Walker, W. H. 1966, Convergence of the Iterative Solution of the Auxiliar Equations for Rayleigh Scattering. Astrophys. J., 144, 798.CrossRefGoogle Scholar
22. Dave, J. V. 1964, Meaning of Successive Iteration of the Auxiliary Equation in the Theory of Radiative Transfer. Astrophys. J., 140, 1292.CrossRefGoogle Scholar
23. Delache, Ph. Comment on the Inversion of the Darkening Law. Astrophys. J., (submitted f. publication).Google Scholar
24. Delache, Ph. 1966, Une Généralisation de l'Approximation de Barbier-Eddington. Ann. Astrophys., 29.Google Scholar
25. Delache, Ph. 1965, C. r. Acad. Sci. Paris, 261, 643646.Google Scholar
26. Delache, Ph. Symp. on Interdisciplinary Asp. of Rad. Transfer, Philadelphia, Feb. 1966.Google Scholar
27. Feautrier, P. 1964, A Procedure for Computing the Mean Intensity and the Flux. Proc. First Havard-Smithson. Conf., Cambridge, p. 80.Google Scholar
28. Feautrier, P. 1964, A Method for Improving the T(x)–Law. Proc. I. Harvard-Smithsot Conf. on Stellar Atmospheres, Cambridge, p. 108.Google Scholar
29. Feautrier, P. 1964, Sur la Résolution Numérique de l'Equation de Transfert. C. r. Acad. Sci. Paris, 258, 3189.Google Scholar
30. Frisch, U. 1967 (unpublished).Google Scholar
31. Gingerich, O., Mihalas, D., Matsushima, S., Strom, S. 1965, An Archetype Non-Grey Stellar Atmosphere. Astrophys. J., 141, 316.CrossRefGoogle Scholar
32. Henyey, L. G. Radiative Transfer, I: The Flux-Temperature Relation and Non-Grey Stellar Atmospheres. Submitted to Astrophys. J. Google Scholar
34. Hoang, Binh-Dy, McCarroll, R. 1966, Méthode Simple de Calcul des Ecarts à l'Equilibre Thermodynamique Local, C. r. Acad. Sci. Paris, 262, 476Google Scholar
35. Horak, H. G., Janousek, A. L. 1965, The H- and Related-Functions for p(cos θ ) = 1 + 1 P 1 (cos θ) + 2 P 2 (cos θ). Astrophys. J. Suppl., 11, 101.CrossRefGoogle Scholar
36. Hummer, D. G. 1965, The Emission Coefficient. Proc. 2nd Harvard-Smithson. Conf. on Stellar Atmospheres, 13.Google Scholar
37. Hummer, D. G. 1966, Introduction to Radiative Transfer Problems in Stellar Atmospheres. Presented at the Symp. on Inter-Disciplinary Aspects of Rad. Energy Transfer, Philadelphia. February.Google Scholar
38. Hummer, D. G. 1964, The Mean Number of Scatterings by a Resonance-Line Photon. Astrophys. J., 140, 276.CrossRefGoogle Scholar
39. Irvine, W. M. 1966, The Distribution of Photon Optical Paths in a Scattering Atmosphere. Astrophys. J., 144, 1140.CrossRefGoogle Scholar
40. Ivanov, V. V. 1965, Scattering of Light in an Atmosphere of Finite Optical Thickness. Sov. Astr. A. J., 8, 874.Google Scholar
41. Ivanov, V. V. 1964, Light Scattering in a Plane Layer. Astr. Zu., 41, 44.Google Scholar
42. Ivanov, V. V. 1964, On the Problem of Light Scattering in the Atmosphere of Finite Optical Thickness. Astr. Zu., 41, 1097.Google Scholar
43. Ivanov, V. V., Leonov, V. V. 1965, Light Scattering in an Optically Thick Atmosphere with a Non-Spherical Indicatrix. Izv. Akad. Nauk, Ser. Phys. Atm., 1, 803.Google Scholar
44. Kalkofen, W. 1966, Deviations from LTE in Stellar Atmospheres. J. quantit. Spectrosc. radiat. Transfer, 6, 633.CrossRefGoogle Scholar
45. King, J. I. F., Sillars, R. V., Harrison, R. H. 1965, Hopf q-Function Evaluated to Eight- Digit Accuracy. Astrophys. J., 142, 1655.CrossRefGoogle Scholar
46. Kogure, T. 1967, The Radiation Field and the Theoretical Balmer Decrement of Be-Stars Publ. astr. Soc. Japan (in preparation).Google Scholar
47. Kolesnik, I. G., Frank-Kemenetsky, D. A. 1964, Analysis of the Energy Distribution near the Balmer Limit in Spectra of Non-Stable Stars. Astr. Zu., 41, 178.Google Scholar
48. Lucy, L. B. 1964, A Temperature Correction Procedure. Proc. First Harvard-Smithson. Conf. on Stellar Atmospheres, p. 93.Google Scholar
49. Mihalas, D., Stone, M. Effects of Departures from LTE on Hydrogen and Helium Continua in Early-Type Stars. In preparation.Google Scholar
50. Mihalas, D. 1966, LTE Model Atmospheres with Line Blanketing: Review and Future Prospects. J.quantit. Spectrosc. radiat. Transfer, 6, 581.CrossRefGoogle Scholar
51. Minin, I. N. 1964, Non-Stationary Radiation Field of a Semi-infinite Medium. Dokl. Akad. Nauk SSSR, 154, 1059.Google Scholar
52. Minin, I. N., Piliposian, A. G., Shidlovskaja, N. A. 1964, Tables of Ambartzumian Functions for Anisotropic Scattering, Trudy astr. Obs. Leningrad. gos. Univ., 20, 12.Google Scholar
53. Nagimer, D. I. 1964, On the Solution of Integral Equations of the Theory of Ligh Scattering. Astr. Zu., 41, 669.Google Scholar
54. Nagimer, D. L, Ivanov, V. V, 1966, Transfer of Resonance Radiation in an Infinite Medium, I. Astrofizika, 2, 5.Google Scholar
55. Nagimer, D. I., Ivanov, V. V. 1966, Transfer of Resonance Radiation in an Infinite Medium, II. Astrofizika, 2.Google Scholar
56. Nikoghossian, A. G. 1965, Polychromatic Diffuse Reflection of Light from an Infinitely Deep One-Dimensional Medium. Astrofizika, 1, 285.Google Scholar
57. Obridko, V. N. 1965, The Matrix of .Radiative Scattering in a Magnetic Field. Astr. Zu., 42, 102.Google Scholar
58. Pavhor, S., Kuščer, I. 1966, On the Non-Uniqueness of Solutions of Chandrasekhar's S-Equation in Radiative Transfer. Astrophys. J., 143, 888.CrossRefGoogle Scholar
59. Pavlov, V. E. 1964, Atmospheric Scatterings Law in the Optical and Ultraviolet Regions of the Spectrum. Astr. Zu., 41, 546.Google Scholar
60. Pavlov, V. E. 1964, Atmospheric Indicatrix of Scattering in the Region of Small and Large Scattering Angles. Astr. Zu., 41, 122.Google Scholar
61. Pecker, J.-C. La Structure de la Photosphère. In: The Solar Spectrum, ed. by Jager, C. de p. 29.Google Scholar
62. Pecker, J.-C. 1965, Model Atmospheres. A. Rev. Astr. Astrophys., 3, 135.CrossRefGoogle Scholar
63. Pecker, J.-C. 1964, Sur une Interprètation possible de la Phase Oscillatoire des Novae. Ann. Astrophys., 27, 287.Google Scholar
64. Rublev, S. V. 1965, Characteristics of the He III Zone in the Atmospheres of the WR Stars. Astr. Zu., 42, 718.Google Scholar
65. Siewert, C. E., Zweifel, P. F. 1966, An Exact Solution of Equations of Radiative Transfer for Local Thermodynamic Equilibrium in the Non-Grey Case. Picket Fence Approximation. Ann. Phys., 36, 61.CrossRefGoogle Scholar
66. Sobolev, V. V. 1964, Diffusion of Radiation in a Plane Layer of Large Optical Thickness. Dokl. Akad. Nauk SSSR, 155, 316.Google Scholar
67. Stewart, J. C. 1966, (unpublished).Google Scholar
68. Stewart, J. C. 1964, Non-Grey Radiative Transfer. Rod. Transfer, 4, 723.Google Scholar
69. Swihart, T. L. 1966, Structure of the Solar Photosphere, I. Blanketing and Convection. Astrophys, J., 143, 358.CrossRefGoogle Scholar
70. Swihart, T. L. 1965, A Modification of the Krook-Avrett Temperature Correction Procedure. Astrophys, J., 141, 821,CrossRefGoogle Scholar
71. Swihart, T, L. 1964, Investigation of the Time-Dependent Heating of a Grey Atmos-phere. Astrophys. J., 139, 772.CrossRefGoogle Scholar
72. Thomas, R. N. 1965, Some Aspects of Non-Equilibrium Thermodynamics in the Presence of a Radiation Field. Univ. of Colorado Press.Google Scholar
73. Thomas, R. N. 1965, Comment on the Difference between Non-LTE and a Pure Absorption Model for the Line Blanketing Effect. Astrophys. J., 141, 333.CrossRefGoogle Scholar
74. Tsuji, T. 1965, Non-grey Model Atmospheres in Radiative Equilibrium. Publ. astr. Soc. Japan, 17, 152.Google Scholar
75. Ueno, S. 1967, Small-Angle Approximation of the Source Function in the Equation of Radiative Transfer. J. atmos. Sci., to be published.Google Scholar
76. Warner, B. 1964, Departures from Local Thermodynamic Equilibrium in the Solar Atmosphere. Mon. Not. R. astr. Soc., 138, 63.CrossRefGoogle Scholar
77. Wildt, R. 1964, Thermodynamics of the Grey Atmosphere, I: Reversible Adiabatic Process. Astrophys. J., 140, 1343.CrossRefGoogle Scholar
78. Wildt, R. 1966, Thermodynamics of the Grey Atmosphere, II: Unattainability of Detailed Balancing. Astrophys. J., 143, 363.CrossRefGoogle Scholar
79. Wilson, S. J., Sen, K. K. 1964, Modified Spherical Harmonic Method for Solving the Equation of Transfer with Anisotropic Scattering. Ann. Astrophys., 27, 46.Google Scholar
80. Wilson, S. J., Sen, K. K. 1964, Modified Spherical Harmonic Method and Spherical Geometry, I. Ann. Astrophys., 27, 654.Google Scholar
81. Yanovitsky, E. G. 1964, The Diffusion of Radiation in a Plane Layer with, Isotropic Scattering. Astr. Zu., 41, 898.Google Scholar
82. Yengibarian, N. B. 1965, On a Non-Linear Problem of Radiative Transfer. Astrofizika, 1, 297.Google Scholar
83. David, K. H. 1965, Näherungen von S (τ), J(τ), und πF(τ), dargestellt durch die Intensitaten auf der Sonnenscheibe. Z. Astrophys., 61, 237.Google Scholar
84. Matsushima, S., Terashita, Y. 1964, Effect of Errors in the Absorption Coefficient on the Non-Grey Model Stellar Atmospheres. Astrophys. J., 140, 285.CrossRefGoogle Scholar
85. Strom, S. E., Kurucz, R. L. 1966, A Statistical Procedure for Computing Line-Blanketed Model Stellar Atmospheres with Applications to the F5 IV Star Procyon. J. quantit. Spectrosc. radiat. Transfer, 6, 591.CrossRefGoogle Scholar
86. Dietz, R. D., House, L. L. 1965, The formation of the Lyman continuum: isotherms) atmosphere, Astrophys. J., 141, 1393.CrossRefGoogle Scholar
87. Mullikin, T. W. 1966, The complete Rayleigh-scattered field within a homogeneous plane-parallel atmosphere. Astrophys. J., 145, 886.CrossRefGoogle Scholar
88. Frisch, H. 1966, The Effect of Line Absorption on the Temperature at the Surface of the Solar Photosphere. J. quantit. Spectrosc. radiat. Transfer, 6, 629.CrossRefGoogle Scholar
89. Gingerich, O. 1966, Blanketing Approximations for Solar Models. J. quantit. Spectrosc radiat. Transfer, 6, 609.CrossRefGoogle Scholar
1. Auman, J. R. Astrophys, J, Suppl. no. 127, (in press).Google Scholar
2. Bély, O. 1965, Extension de la théorie généralisée du défaut quantique au cas des ions hydrogénoïdes I, II. Ann. Astrophys., 28, 567 and 843.Google Scholar
3. Bode, G. 1965, Die kontinuierliche Absorption von Sternatmosphären. Sonderdruck, Kiel.Google Scholar
4. Burgess, A. 1965, Dielectronic Recombination in the Corona. Ann. Astrophys., 28, 774.Google Scholar
5. Buslavsky, V. G. 1964, On the Sources of Opacity in the Atmospheres of Late-Type Stars. Vestnik Leningrad, gos. Univ., 13, 114.Google Scholar
6. Cox, A. N., Stewart, J. N. 1965, Radiative and Conductive Opacities for Eleven Astrophysical Mixtures. Astrophys. J. Suppl., II, 94.Google Scholar
7. Doughty, N. A., Fraser, P. A., McEachran, R. P. 1966, The Bound-Free Absorption Coefficient of the Negative Hydrogen Ion. Mon. Not. R. astr. Soc., 132, 255.CrossRefGoogle Scholar
8. Doughty, N. A., Fraser, P. A. 1966, The Free-Free Absorption Coefficient of the Negative Hydrogen Ion. Mon. Not. R. astr. Soc., 132, 267.CrossRefGoogle Scholar
9. Goldberg, L., Dupree, A. K., Allen, J. W. 1965, Collisional Excitation of Autoionizing Levels. Ann. Astrophys., 28, 585.Google Scholar
10. John, T. L. 1964, The Free-Free Transitions of the Negative Hydrogen Ion in the Exchange Approximation. Mon. Not. R. astr. Soc., 128, 93.CrossRefGoogle Scholar
11. John, T. L. 1966, The Free-Free Transitions of an Electron in the Field of a Hydrogen Atom at Infra-red Frequencies. Mon. Not. R. astr. Soc., 131, 315.CrossRefGoogle Scholar
12. John, T. L. 1966, The Limiting Behaviour of the Absorption Cross Sections of the Negative Hydrogen Ion. Mon. Not. R. astr. Soc., 133, 447.CrossRefGoogle Scholar
13. Kandel, R. 1966, L'absorption continue de l'ion négatif du chlore. C. r. Acad. Sci. Paris, 362, 373.Google Scholar
14. McCarrol, R., Salin, A. 1966, L'excitation de l'hydrogéne par protons. Ann. Astrophys., 29. 283.Google Scholar
15. McDowell, M. R. C., Williamson, J. H., Myerscough, V. P. 1966, Continuous He Absorption. Astrophys. J., 144, 827.CrossRefGoogle Scholar
16. Peach, G. 1965, A General Formula for the Calculation of Absorption Cross-Sections for Free-Free Transitions in the Field of Positive Ions. Mon. Not. R. astr. Soc., 130, 361.CrossRefGoogle Scholar
17. Praderie, F. 1964, Calcul de quelques sections de photoionisation du carbone neutre. Ann. Astrophys., 27, 129.Google Scholar
18. Rensbergen, W. van 1967, The Influence of Doubly Excited Levels on the Ionization Formula for the Solar Corona. Solar Physics, 1 (in press).Google Scholar
19. Sommerville, W. B. 1965, The Continuous Absorption Coefficient of He . Astrophys. J., 141, 811.CrossRefGoogle Scholar
20. Vardya, M. S. 1964, Opacity at λ 1.65μ in Late-Type Stars. Proc. 1st Harvard-Smith- sonian Conf., p. 50.Google Scholar
21. Vardya, M.S. 1964, Atmospheric Rosseland Mean Absorption Coefficients. Astrophys. J., 8, 277.CrossRefGoogle Scholar
22. Vardya, M. S., Böhm, K.-H. 1965, Pressure Broadening and Opacity in the M2 V star HD 95735. Mon. Not. R. astr. Soc., 131, 89.CrossRefGoogle Scholar
23. Vardya, M. S. 1965, A Method for Estimating H2O Absorption. J. quantit. Spectrosc. radiat. Transfer, 5, 867.CrossRefGoogle Scholar
24. Vardya, M. S. 1966, Negative Chlorine Ion and M-Spectral Type Stars. Mon. Not. R. astr. Soc., 132, 475.CrossRefGoogle Scholar
25. Vardya, M. S. 1966, Simplified Description of the Line Absorption Coefficient in Blanketing Effect Computation. J. quantit. Spectrosc. radiat. Transfer, 6, 539.CrossRefGoogle Scholar
26. Vardya, M. S. 1967, Role of Negative Ions in Late-Type Stars. Mem. R. astr. Soc. (in press).Google Scholar
27. Vardya, M. S. 1966, March with Depth of Molecular Abundances in the Outer Layers of K and M Stars. Mon. Not. R. astr. Soc., 134, 347.CrossRefGoogle Scholar
28. Vardya, M. S. 1967, Sources of Opacity in Late-Type Stars, a Review. Prec. of the IAU Symp. on Late-Type Stars (in press).Google Scholar
29. Kodaira, K. 1965, Quantitative Analyse des Intensitätssprunges im Sonnenspektrum bei λ 2085 Å. Z. Astrophys., 60, 340.Google Scholar
30. Gingerich, O. 1964, Review of Opacity Calculations. Proc. 1st Harvard-Smiths. Conf. on Stellar Atmosph., p. 17.Google Scholar
31. Baerentzen, J., Mikkelsen, E. 1967, Unpublished.Google Scholar
32. Ohmura, T. 1964, Evaluation of free-free absorption coefficient of the negative ion. Astrophys, J., 140, 282.CrossRefGoogle Scholar
33. Peach, G. 1966, Total Continuous Absorption Coefficients for Complex Atoms. Preprint.CrossRefGoogle Scholar
34. Myerscough, V. P. 1966, Unpublished.Google Scholar
35. Schlüter, D. 1965, Die Berechnung der Übergangswahrscheinlichkeiten von Serien-grenzkontinua mit Anwendung auf die schweren Edelgase. Z. Astrophys., 61, 67.Google Scholar
36. Weinberg, M., Berry, R. S. 1966, Forbidden Continuum: Free-Bound Transitions in Hydrogen Plasmas. Phys. Rev., 144, 75.CrossRefGoogle Scholar
1. Baglin, A, 1964, Condition d'existence d'une zone convective dans une atmosphère soumise au triage gravitationnel. Ann. Astrophys., 27, 389.Google Scholar
2. Baerentzen, J. 1965, The Adiabatic Temperature Gradient and the Specific Heat c p in the Outer Hydrogen-Helium Convection Zones. Z. Astrophys., 62, 221.Google Scholar
3. Bird, G. A. 1965, The Equilibrium State of a Shock-heated Atmosphere. Astrophys. J., 141. 1455.CrossRefGoogle Scholar
4. Böhm, K.-H. 1967, The Outer Solar Convection Zone, in Proc. IAU Symp. no. 28 ‘Aerodynamics in Stellar Atmospheres’ (in press).Google Scholar
5. Böhm, K.-H. 1964, Significance of Uncertainties in the Physical Theory of Radiative Transfer. Proc. 1st Harvard-Smiths, Conf. on Stellar Atmosph., p. 155.Google Scholar
6. Böhm, K.-H. 1966, Die Lithiumhäufigkeit und die Struktur der äusseren Konvektions zone in sonnenähnlichen Sternen. Z. Naturforschung, 21a, 1107.CrossRefGoogle Scholar
7. Detnzer, W. 1965, On the Magneto-Hydrostatic Theory of Sunspots. Astrophys. J., 141, 548.CrossRefGoogle Scholar
8. Edmonds, F. N. Jr, 1966, A Coherence Analysis of Fraunhofer-line Fine Structure an Continuum Brightness Fluctuations near the Centre of the Solar Disk, II. Astrophys. J., 144. 733.CrossRefGoogle Scholar
9. Edmonds, F. N. Jr, McCullough, J. R. 1966, The Evidence for an Oscillatory Com ponent in Solar Granulation Brightness Fluctuations. Astrophys. J., 144, 754.CrossRefGoogle Scholar
10. Faulkner, J., Griffiths, K., Hoyle, F. 1965, On the Surface Boundary Conditions for Stars. Mon. Not. R. astr. Soc., 129, 363.CrossRefGoogle Scholar
11. Frisch, U. 1964, Couplage d'ondes magnétodynamiques en milieu stratifié. Ann. Astrophys., 27, 224.Google Scholar
12. Gough, D. O., Taylor, R. J. 1966, The Influence of a Magnetic Field on Schwarzschild Criterion for Convective Instability in an Ideally Conducting Fluid. Mon. Not. R. astr. Soc., 133, 85.CrossRefGoogle Scholar
13. Henyey, L. G. Vardya, M. S., Bodenheimer, P. 1965, The Calculation of Mode Envelopes. Astrophys. J., 142, 841.CrossRefGoogle Scholar
14. Hollandsky, O. P. 1964, Sound Velocities in the Atmospheres of Hot Supergiants Publ, Krym. astrofiz. Obs., 32, 127.Google Scholar
15. Hollandsky, O. P. 1965, On Supersonic Turbulence in the Atmospheres of Hot Super giants. Publ. Krym. astrofiz. Obs., 33, 266.Google Scholar
16. Hollandsky, O. P., Chub, A. T. 1966, Investigation of the Turbulent Spectrum in Application to Stellar Atmospheres. Publ. Krym. astrofiz. Obs., 35, 34.Google Scholar
17. Kaplan, S. A., Petrukhin, N. S. 1965, On the Theory of Convection in a Polytropi Atmosphere with a Uniform Magnetic Field. Astr. Zu,, 42, 74.Google Scholar
18. Kato, S. 1966, The Effect of Compressibility upon Oscillatory Convection. Publ. astr. Soc. Japan, 18.Google Scholar
19. Kato, S. 1966, On the Atmospheric Oscillations Excited by Turbulence. Astrophys. J., 143, 372.CrossRefGoogle Scholar
20. Kato, S. 1966, The Response of an Unbounded Atmosphere to a Point Disturbance, I. Time-Harmonic Disturbances. Astrophys. J., 143, 893.CrossRefGoogle Scholar
21. Kato, S. 1966, The Response of an Unbounded Atmosphere to Point Disturbances, II. Impulsive Disturbances. Astrophys. J., 144, 326.CrossRefGoogle Scholar
22. Kopylov, I. M. 1964, Turbulent Motions in Stellar Atmospheres, in Problems of Magneto-hydrodynamics and Cosmic Gas Dynamics, pp. 74106, Fizmatgiz Publ. Co., Moscow.Google Scholar
23. Kuhi, L. V. 1964, Mass loss from T Tauri Stars. Astrophys. J., 140, 1409.CrossRefGoogle Scholar
24. Lemaire, J. 1966, Evaporative and Hydrodynamical Atmospheric Models. Ann. Astrophys., 29, 197.Google Scholar
25. Lighthill, M. I. 1967, Waves in the Sun's Atmosphere in Proc. IAU Symposium no. 28, Aerodynamic Phenomena in Stellar Atmospheres (in press).Google Scholar
26. McLean, D. 1964, Le champ magnétique dans un fluide de conductivité infinie placé dans un champ gravitationnel uniforme. Ann. Astrophys., 27, 195.Google Scholar
27. Mein, P. 1966, Champ macroscopique des vitesses dans l'atmosphère solaire, d'après les mesures de déplacement des raies de Fraunhofer. Ann. Astrophys., 29, 153.Google Scholar
28. Meyer, F., Schmidt, H. U. 1966, Response of Solar Atmosphere to granular disturbance, Trans. IAU, 12B, 559. See also Z. Astrophys., 65, 274.Google Scholar
29. Mihalas, D. 1965, Constant Flux Convective Models Atmospheres. Astrophys. J., 141, 564.CrossRefGoogle Scholar
30. Miyamoto, S. 1965, Thermal Stability of the Chromosphere and Spicule. Publ. astr. Soc. Japan, 17, 127.Google Scholar
31. Moore, D. W. 1967, Penetrative Convection, in Proc. IAU Symposium no. 28, Aerodynamic Phenomena in Stellar Atmospheres(in press).Google Scholar
32. Moore, D. W., Spiegel, E. A. 1966, A Thermally Excited Non-linear Oscillator. Astrophys. J., 143, 871.CrossRefGoogle Scholar
33. Nissen, P. E. 1965, Turbulence in the Solar Photosphere as derived from the Study of Centre-to-Limb Variations of Equivalent Widths of Ti 1 Lines. Ann. Astrophys., 28, 556.Google Scholar
34. Olson, E. C. 1966, The Depth Dependence of Solar Turbulence. Astrophys. J., 143, 912.CrossRefGoogle Scholar
35. Olson, E. C. 1966, The Effect of Acoustic Waves and Convection on Solar Line Asym-metries. Astrophys. J., 143, 904.CrossRefGoogle Scholar
36. Rublev, S. V. 1964, On the Dynamic State of the Atmospheres of WR Stars. Astr. Zu., 41, 1063.Google Scholar
37. Sack, N. 1967, Studies in detailed numerical techniques for the fitting of a radiative zone to a convection zone. Ann. Astrophys., (in press).Google Scholar
38. Saito, M. 1965, On Shock, Propagation and the Chromospheric Structure of Late-Type Stars. Publ. astr. Soc. Japan, 17, 107.Google Scholar
39. Schatzman, E. 1967, Convective Transport of Elements Formed at the Surface of the Stars and their Dilution in the Convection Zone. Unpublished.Google Scholar
40. Sitnik, G. F. 1963, Stability Criterion for Hydrostatic Equilibrium. Astr. Zu., 40, 413.Google Scholar
41. Souffrin, P. 1966, Hydrodynamique d'une atmosphère perturbée par une zone convective sous-jacente. Ann. Astrophys., 29, 55.Google Scholar
42. Spiegel, E. A. 1965, Convective Instability in a Compressible Atmosphere, I. Astrophys J., 141, 1068.CrossRefGoogle Scholar
43. Spiegel, E. A. 1966, Energy Transport by Turbulent Convection. In Stellar Evolution (eds. Cameron, A. G. W., Stein, R. F.) Plenum Press, New York.Google Scholar
44. Spiegel, E. A. 1967, The Theory of Turbulent Convection. Proc. IAU Symposium, no. 28: Aerodynamic Phenomena in Stellar Atmospheres (in press).Google Scholar
45. Swihart, T. L., Margrave, T. E. 1967, Inhomogeneities in the solar photosphere. Unpublished.Google Scholar
46. Uchida, Y. 1965, Standing Mode of Compressional-body Gravity Wave in the Solar Chromosphere. Astrophys. J., 142, 335.CrossRefGoogle Scholar
47. Walter, K. 1965, Geordnete Strömungen in instabilen Schichten grosser Ausdehnung mit Anwendung auf stellare Konvektionszonen. Ann. Astrophys., 28, 648.Google Scholar
48. Weiss, N. O. 1964, Magnetic flux tubes and convection in the Sun. Man. Not. R. astr. Soc., 128, 225.CrossRefGoogle Scholar
49. Weiss, N. O. 1966, The Expulsion of Magnetic Flux by Eddies. Proc. R. Soc. London, Ser. A, 293, 310.Google Scholar
50. Weytnann, R., Sears, R. L. 1965, The Depth of the Convective Envelope on the Lower Main Sequence and the Depletion of Lithium. Astrophys. J., 143, 174.Google Scholar
51. Wilson, O. C. 1966, Stellar Convection Zones, Chromospheres, and Rotation. Astrophys. J., 144, 695.CrossRefGoogle Scholar
52. Yamaguchi, S. 1967, Convective Instability in a Layer of Varying Superadiabatic Gradient. Publ. astr. Soc. Japan. (in press).Google Scholar
53. Zirker, J. B. 1964, On the Periods of Large-Amplitude Photospheric Oscillations. Ann. Astrophys., 27, 429.Google Scholar
54. Grover, R., Hardy, J. W. 1966, The propagation of shocks in exponentially decreasing atmospheres. Astrophys. J., 143, 48.CrossRefGoogle Scholar
55. Kohl, K. 1966, Das Eindringen von Strömungen in die stabile Schicht unterhalb der solaren Wasserstoffkonvektionszone. Z. Astrophys., 64, 472.Google Scholar
56. Frazier, E. N. 1966, An Observational Study of the Hydrodynamics of the Lower Solar Atmosphere. Thesis, Berkeley.CrossRefGoogle Scholar
57. Kuperus, M. 1965, The Transfer of Mechanical Energy in the Sun and the Heating of the Corona. Thesis, Utrecht.Google Scholar
1. Dolan, J. F. 1965, Stellar molecular abundances, I. Polyatomic molecules. Astrophys. J., 142, 1621.CrossRefGoogle Scholar
2. Kolesnik, I. G. 1965, Enhancement of ionization equilibrium in a stellar atmosphere, Astr. Zu., 42, 63.Google Scholar
3. Schlender, B., Traving, G. 1965, Tschebycheff-Approximation von Zustandssummen, Z. Astrophys., 61, 92.Google Scholar
4. Souffrin, S. 1965, Influence des collisions inélastique sur la fonction de distribution des eléctrons dans des conditions astrophysiques. Arm. Astrophys., 28, 399.Google Scholar
5. Traving, G., Baschek, B., Holweger, H. 1966, Tabellen für die Berechnung von Zustandssummen. Abh. Hamburger Sternwarte, 8, Nr. 1.Google Scholar
6. Tsuji, T. 1964, Molecular Abundance in Stellar Atmospheres. Ann; Toyko astr. Obs., 9. 1.Google Scholar
7. Vardya, M. S. 1964, Pressure Dependent Partition Functions and Equilibrium Constants for Molecular Hydrogen. Proc. 1st Harard Smithsonian Conf. on Stellar Atmospheres, P. 5.Google Scholar
8. Vardya, M. S. 1965, Thermodynamics of a Solar Composition Gaseous Mixture. Mon. Not. R. astr. Soc., 129, 205.CrossRefGoogle Scholar
9. Vardya, M. S. 1965, Pressure Dissociation and Molecular Hydrogen. Mon. Not. R. astr. Soc., 129, 345.CrossRefGoogle Scholar
10. Wyller, A., Morris, S. 1967 (submitted to Ann. Astrophys.).Google Scholar
1. Brandt, J. C. 1966, Chemical composition of the photosphere and corona as influenced by the solar wind. Astrophys. J., 143, 265.CrossRefGoogle Scholar
2. Gorbatzky, V. G. 1965, On the Influence of Electron Collisions of Balmer Line Intensities in Spectra of Moving Stellar Envelopes. Astrofizika, 1, 129.Google Scholar
3. Hughes, C. J. 1965, Profiles of Lyman-Alpha scattered by free electrons in the solar corona. Astrophys. J., 142, 321.CrossRefGoogle Scholar
4. Locoarret, M. 1965, Enveloppes d'étoiles Be: variations spectrales et caractéristiqu physiques. Ann. Astrophys., 28, 321.Google Scholar
5. Livshitz, M. A. 1963, An Estimate of the Electron Densities in Stellar Chromosphere Astr. Zu., 40, 1065.Google Scholar
6. Livshitz, M. A., Nikolsky, G. M. 1964, The n θ-Trelation in the Transition Regio between the Chromosphere and Corona. Astr. Zu., 41, 75.Google Scholar
7. Magnan, Chr. 1965, Les Couches Extérieures de la Composante de Type K de 31 Cygr Ann. Astrophys., 28, 512.Google Scholar
8. Athay, R. G. 1966, Radiative Energy Loss from the Solar Chromosphere and Coron Astrophys. J., 146, 223.CrossRefGoogle Scholar
1. Abhyankar, K. D. 1964, On the Schuster Problem for a Moving Atmosphere. I, II. Astrophys. J., 140, 1353, 1368.Google Scholar
2. Abhyankar, K. D. 1965, On the Schuster Problem for a Moving Atmosphere, III. Astrophys. J.,141, 1056.CrossRefGoogle Scholar
3. Athay, R. G. 1964, Source-Function Equality in Multiplete. Astrophys. J., 140, 1579.CrossRefGoogle Scholar
4. Atha, R. G. 1965, Theoretical Line Intensities. I. Strong Emission Lines. II. Excitation of Chromospheric He II and Hydrogen. III. Solar UV Lines and Continua of H, He I, and He II and the Chromospheric Model. Astrophys. J., 142, 724, 732, 755.Google Scholar
5. Athay, R. G. 1966, Theoretical Line Intensities. IV. Source Functions and Equivalent Widths. Astrophys. J., 144, 1159.CrossRefGoogle Scholar
6. Avrett, E. H. 1965, Solutions of the Two-Level Line Transfer Problem with Complete Redistribution. Proc. 2nd Harvard-Smithson. Conf. on Stellar Atmospheres, p. 101.Google Scholar
7. Avrett, E. H., Hummer, D. G. 1965, Non-coherent Scattering, II: Line Formation with a Frequency Independent Source Function. Mon. Not. R. astr. Soc., 130, 295.CrossRefGoogle Scholar
8. Balli, E., Kiral, A., Pecker, J.-C. 1965, Abaque pour le calcul des profondeurs de formation. Publ. Istanbul. Univ. Obs., no. 83.Google Scholar
9. Baschek, B., Holweger, H., Traving, G. 1966, Ein Algol-Programm für die Analyse von Sternspektren. Abh. Hamburger Sternwarte, 8, no. 1.Google Scholar
10. Baschek, B., Traving, G. 1964, Differentielle Wachstumskurven. Z. Astrophys., 59, 276.Google Scholar
11. Böhm-Vitense, E. 1965, A Differential Equation Solution of the Non-LTE Line Transfer Problem. Proc. 2nd Harvard-Smithson. Conf. on Stellar Atmospheres, p. 165.Google Scholar
12. Chiarella, C., Reichel, A. 1966, On the Evaluation of Voigt Spectral Line Functions. Mon. Not. R. astr. Soc,, 134, 83.CrossRefGoogle Scholar
13. Cuny, Y. 1967 (in preparation).Google Scholar
14. Dumont, S. 1966, C. r. Acad. Sci. Paris, 262, 740.Google Scholar
15. Dumont, S. 1966, C. r. Acad. Sci. Paris, 263, 85 Google Scholar
16. Edmonds, F. N., Schlüter, H., Wells, D. C. 1967, Hydrogen-Line Stark Broadening Functions. Mem. R. astr. Soc., (in press).Google Scholar
17. Edmonds, F. N. 1967 (work in progress).Google Scholar
18. Gökdoǧan, N., Pecker, J.-C. 1964, Note sur I'utilisation des courbes de croissance, Ann. Astrophys., 27, 417.Google Scholar
19. Goldberg, L. 1964, The Origin of the Emission Reversals in the Fraunhofer H- and K-Lines. Astrophys. J., 140, 384.CrossRefGoogle Scholar
20. Hummer, D. G. 1965, General Noncoherent Scattering. Proc. 2nd Harvard Smithson. Conf. on Stellar Atmospheres, p. 143.Google Scholar
21. Hummer, D. G., Rybicki, G. B. 1966, Non LTE Line Formation with Spatial Variations of the Doppler Width. J. quantit. Spectrosc. radiat. Transfer, 6, 661.CrossRefGoogle Scholar
22. Hummer, D. G., Rybicki, G. B. 1967, Computational Methods for Non-LTE Line-Transfer Problems. In Method in Computational Physics, 7, Academic Press (in press).Google Scholar
23. Hummer, D. G., Stewart, J. C. 1967, Thermalization Lengths and the Homogeneous Transfer Equation in Line Formation. Submitted to Astrophys. J. CrossRefGoogle Scholar
24. Ivanor, V. V., Nagirner, D. I. 1965, H-functions in the Theory of Transfer of Resonance Radiation. Astrofizika, 1, 143.Google Scholar
25. Jefferies, J. T. 1965, Multilevel Problems. Proc. 2nd Harvard-Smithson. Conf. on Stellar Atmospheres, p. 177.Google Scholar
26. Johnson, H. R. 1964, A Theoretical Study of the Excitation of Sodium in the Solar Photosphere. Ann. Astrophys., 27, 695.Google Scholar
27. Johnson, H. R. 1965, Sodium Equilibrium and the NaD Lines. Proc. 2nd Harvard-Smithson. Conf. on Stellar Atmospheres, Spec. Report, 174, 333.Google Scholar
28. Johnson, H. R., Klinglesmith, D. 1965. The Coupled Line Transfer Problem for Hydrogen. Proc. 2nd Harvard Smithson. Conf. on Stellar Atmospheres, p. 221.Google Scholar
29. Kurochka, L. N. 1965, Electron Density Determination based on Emission Balmer Lines. Astrofizika, 1, 369.Google Scholar
30. Kurochka, L. N. 1966, Doppler-Effect and the Last Resolved Balmer Line. Astrofizika, 2, 131.Google Scholar
31. Mugglestone, D., O'Mara, B. I. 1965, Saturation Effects in Stellar Atmospheric Absorption Lines. Mon. Not. R. astr. Soc., 129, 41.CrossRefGoogle Scholar
32. Mugglestone, D., O'Mara, B. I. 1966, The Influence of Stark Broadening on Abundance Determinations. Mon. Not. R, astr. Soc., 132, 87.CrossRefGoogle Scholar
33. Nagirner, D. I. 1964, On the Solution of Integral Equations of the Theory of Light Scattering. Astr. Zu., 41, 669.Google Scholar
34. Nagirner, D. I., Ivanov, V. V, 1966, Transfer of Resonance Radiation in an Infinite Medium, I, II. Astrofizika, 2, 5 and 2, no. 2.Google Scholar
35. Obridko, V. N. 1965, The Matrix of Radiative Scattering in a Magnetic Field. Astr. Zu., 42, 102.Google Scholar
36. Obridko, V. N. 1965, Formation of Solar Absorption Lines with a Split upper Level in the Presence of a Magnetic Field. Astr. Zu., 42, 502.Google Scholar
37. Pagel, B. E. J. 1964, R. Obs. Bull., no. 87.Google Scholar
38. Pfennig, H. 1966, Comparison of Quasistatic Line Profiles with Measurements of Balmer and Paschen Hydrogen Lines and Lines of the Diffuse Series of Neutral Helium. J. quantit. Spectrosc, radiat. Transfer, 6, 549.CrossRefGoogle Scholar
39. Pfennig, H., Trefftz, E., Vidal, C. R. 1966, A Critical Note on the up to now Available Stark Broadening Theories of Hydrogen. J. quantit. Spectrosc. radiat. Transfer, 6, 557.CrossRefGoogle Scholar
40. Rachkowski, D. N. 1963, Theory of Formation of Absorption Lines in the Presence of a Magnetic Field. Publ Krym. astrofiz. Obs., 30, 267.Google Scholar
41. Schatzman, E. 1965, Mesures absolues des durés de vie d'états excités. But et méthodes. Ann, Astrophys., 28, 111.Google Scholar
42. Thomas, R. N. 1965, Some Aspects of Non-Equilibrium Thermodynamics in the Presence of a Radiation Field. Univ. of Colorado Press.Google Scholar
43. Thomas, R. N. 1965, Computation of the Line Source Function: A Review of the Physical Problem. Proc. 2nd Harvard-Smithson. Conf., p. 71.Google Scholar
44. Traving, G. 1964, Über die Bildung von Fraunhoferlinien in turbulenten Sternatmosphären. Z. Astrophys., 60, 167.Google Scholar
45. Unno, W., Yamashita, Y. 1966, On Curves of Growth for Line Profiles Truncated at Artificial Continuous Levels. In The Solar Spectrum (ed. by Jager, C. de), p. 102.Google Scholar
46. Van Regemorter, H., Bréchot, S. 1964, L'élargissement des raies spectrales par chocs, I et II, Arm. Astrophys., 27, 432, 739.Google Scholar
47. Van Regemorter, H. 1965, Spectral Line Broadening. Ann. Rev. Astr. Astrophys., 3, 71.CrossRefGoogle Scholar
49. Vidal, C. R. Determination of Electron Densities from Line Merging. J. quantit. spectrosc. radiat. Transfer, 6, 575, 1966.CrossRefGoogle Scholar
50. Waddell, J. III 1964, Reply to Athay's paper: ‘Source Function Equality in Multiplets’. Astrophys. J., 140, 1586.CrossRefGoogle Scholar
51. Wright, K. O. 1966, Stellar Atmospheres and their Spectra. J. R. Astr. Soc. Can., 60, 97.Google Scholar
52. Yamashita, Y. 1964, A Theoretical Study on the Curve of Growth, II. Publ. astr. Soc. Japan, 16, 77.Google Scholar
53. Hummer, D. G. 1964, The Mean Number of Scattering by a Resonance-Line Photon. Astrophys. J., 140, 276.CrossRefGoogle Scholar
54. Averett, E. H. 1966, Source Function Equality in Multiplets. Astrophys. J., 144, 59.CrossRefGoogle Scholar
55. Peytremann, E. 1966, Obs. de Genève, Unpublished.Google Scholar
1. Adams, T., Morton, D. C. In preparation.Google Scholar
2. Audouze, J. 1967, unpublished.Google Scholar
3. van't Veer, F. Modèles empiriques d'atmosphères stellaires. I. Introduction et premièr application; II. Étude statistique, modèle d'une tache solaire; III. Comparaison der différents modèles pour les taches solaires. 1966, Ann. Astrophys., 29, 7, 119; and 223.Google Scholar
4. Auman, J. R. 1966, Model Stellar Atmosphere with T eff = 2500°K. Paper presented at IAU Sym. on Late-Type Stars, Trieste.Google Scholar
5. Baschek, B. 1966, On the Influence of Surface Gravity on UBV Colours of G-Type Stars. J. quantit. Spectros'c. radial. Transfer, 6, 701.CrossRefGoogle Scholar
6. Baschek, B., Holweger, H., Namba, O., Traving, G. 1967, Quantitative Analyse des Spektrums des F8-Sterns Beta Virginis. Z. Astrophys., 65, 418.Google Scholar
7. Baschek, B., Kegel, W., Bode, G., Kodaira, K., Kohl, K., Traving, G. 1964, Quantitative , Interpretation of Stellar Spectra using Model Atmospheres. Proc. 1st Harvard-Smithson. Conf. on Stellar Atmospheres, p. 254.Google Scholar
8. Baschek, B., Oke, J. B. 1965, Effective Temperatures and Gravities of Ap, Am, and Normal A-Type Stars. Astrophys. J., 141, 1404.CrossRefGoogle Scholar
9. Baylac, M.-O. 1966, In preparation.Google Scholar
10. Bernas, R., Gradstajn, E., Reeves, H., Schatzman, E. 1967, On the Nucleosynthesis of Lithium, Beryllium and Boron. Ann, Phys., New York (to be published).Google Scholar
11. Böhm, K.-H., Deinzer, W. 1965, Atmospharen von Zentralsternen planetarischer Nebel, I, Z, Astrophys., 61, 1.Google Scholar
12. Böhm, K.-H., Deinzer, W. 1966, Modellatmosphären für die O'Dell-und die Harman-Seaton-Sequenz. Z. Astrophys., 63, 177.Google Scholar
13. Böhm-Vitense, E., Pyper, D. M., Wallerstein, G. 1964, Spectrum of γ Pegasi between 3300 and 3030Å. Astrophys. J., 140, 807.CrossRefGoogle Scholar
14. Böhm-Vitense, E. 1966, Spectral Analysis by means of the Hydrogen Lines. Struve Memorial Volume, Ed. Herbig, G. (in press).Google Scholar
15. Buslavsky, V. G. 1964, Spectral Energy Distribution of Late-Type Stars. Astr. Zu., 41,631.Google Scholar
16. Cayrel, G. 1966, Analyse détaillée des atmosphères de sept étoiles K. Ann. Astrophys., 29, 413.Google Scholar
17. Chevalier, Cl. Critical Analysis of the Peculiar Abundances in Sirius A. To be published in Ann. Astrophys. Google Scholar
18. Collins, G. W. II 1965, Continuum Emission from a Rotating Non-grey Stellar Atmosphere. Astrophys. J., 142, 265.CrossRefGoogle Scholar
19. Collins, G. W. II, Harrington, J. P. 1966, Theoretical H-Beta Line Profiles and Related Parameters for Rotating B-Stars. Astrophys. J., 146, 152.CrossRefGoogle Scholar
20. Conti, P. S., Wallerstein, G., Wing, R. F. 1965, The Composition of Main-Sequence Stars of Types A-K in the Hyades Cluster. Astrophys. J., 142, 999.CrossRefGoogle Scholar
21. Fischel, D. 1964, On the Influence of the Chemical Composition on the Structure and Metal Index of Stellar Atmospheres. Astrophys. J., 140, 221.CrossRefGoogle Scholar
22. Edmonds, F. N. 1964, A Set of Non-Grey Model Atmospheres for Procyon. Astrophys. J., 140, 902.CrossRefGoogle Scholar
23. Edmonds, F. N. 1966, The Determination of the Ultraviolet Continuum of Procyon from Balmer Line Profiles. Proc. IAU Symposium no. 26, Abundance Determination in Stellar Spectra, p. 159.Google Scholar
24. Edmonds, F. N., Talbert, F. D. 1966, A Spectroscopic Analysis of Procyon, II. The Continuous Spectrum and Line Blanketing. Astrophys. J., 146, 1.Google Scholar
25. Fredrich, L. W., Johnson, H. R., Fay, T. 1966, Infrared Spectroscopy with a Mica Window Tube. Adv. Electronics Electron Phys., 22; Astr. J., 71, 384.Google Scholar
26. Fujita, Y., Tsuji, T. 1966, Some Problems Related to the Chemical Abundance in Cool Stars. Proc. IAU Symposium, no. 26 (Academic Press).Google Scholar
27. Gasson, R. E. M. 1966, Thesis, Cambridge Univ.Google Scholar
28. Gasson, R. E. M., Pagel, B. E. J. 1966, Observatory, 86, 196.Google Scholar
29. Gingerich, O. 1966, Limb Darkening for a Grid of Stellar Atmospheres. Astrophys. J., 144, 1213.CrossRefGoogle Scholar
30. Gökdoğan, N., Pecker, J.-C. 1964, Note sur l'utilisation des courbes de croissance. Ann, Astrophys., 27, 417.Google Scholar
31. Guillaume, C., van Rensbergen, W., Underhill, A. B. 1965, The Theoretical Near Ultraviolet Spectrum of a B2 Star. Bull. astr. Inst. Netherl., 18, 106.Google Scholar
32. Hardorp, J., Strittmatter, P. 1967 (in preparation).Google Scholar
33. Henry, R. C, Mihalas, D. 1964, The Abundance of Magnesium in the Atmospheres of O and B Stars. Astrophys. J., 140, 873.Google Scholar
34. Herbig, G. H. 1965. Lithium Abundances in F5-G8 Dwarfs. Astrophys. J., 141, 588.CrossRefGoogle Scholar
35. Houziaux, L. 1964, Sur la possibilité d'observer les raies de Lyman dans les étoiles du type voisin de Ao V. C. r. Acad. Sci. Paris, 358, 3635.Google Scholar
36. Houziaux, L. 1965, Les raises de Lyman dans le spectre des étoiles B de la séquence principale. C. r. Acad. Sci. Paris, 260, 420.Google Scholar
37. Houziaux, L. 1966, Profil du triplet de O I à 7772 Å dans le spectre de Véga, C. r. Acad. Sci. Paris, 263, 118.Google Scholar
38. Kalkofen, W., Strom, S. E. 1966, The Effects of Deviations from LTE and Line Blanketing on Stellar Atmospheres in the Range B5 to A5. J. quantit. Spectrosc. radiat. Transfer, 6, 653.CrossRefGoogle Scholar
40. Kohl, K. 1964, Die Atmosphäre des Siriua. Z. Astrophys,, 60, 115.Google Scholar
41. Kolesov, A. K. 1964, Continuous Spectra of White Dwarfs. Astr. Zu., 41, 240,Google Scholar
42. Kopylov, I. M. 1966, Electron Densities in the Atmospheres of Hot Stars, II. Publ Krym. astrofiz. Obs., 35, 11. Google Scholar
43. Matsushima, S. 1967, Non-Grey Model Atmospheres for Solar Type Stars, I. The Role of the Hydrogen Molecules as a Source of Continuous Opacity. Submitted to Am. Astrophys. Google Scholar
44. Matsushima, S., Terashita, Y. 1967, Non-Grey Model Atmospheres of Solar Type Stars, II. The Source of Opacity in the Ultraviolet Continuum and its Effect on the Radiation Field in other Spectral Regions. Submitted to the Ann. Astrophys. Google Scholar
45. Mihalas, D. 1965, Model Atmospheres and Line Profiles for Early-Type Stars. Astrophys. J. Suppl., 9, 321.CrossRefGoogle Scholar
46. Mihalas, D. 1965, A Spectroscopic Estimate of the Atmospheric Properties of O and B Stars. Astrophys. J., 140, 885.CrossRefGoogle Scholar
47. Mihalas, D. 1966, Balmer-Line-blanketed Model Atmospheres for A-Type Stars. Astrophys. J. Suppl., 13, 1.CrossRefGoogle Scholar
48. Mihalas, D. 1967 (submitted to Astrophys. J.). Google Scholar
49. Cowley, C. R., Cowley, A. P. 1966, Selection of Data for Abundance Determinations. Proc, IAU Symposium no. 26, p. 43 (Academic Press).Google Scholar
50. Mihalas, D., Morton, D. C. 1965, A Model for a BI V Star with Line Blanketing. Astrophys. J., 142, 253. CrossRefGoogle Scholar
51. Mihalas, D. 1967, Statistical-Equilibrium Model Atmospheres for Early-Type Stars, I. Hydrogen Continua. Submitted to the Astrophys. J. CrossRefGoogle Scholar
52. Morton, D. C. 1964, The X-ray Emission of Neutron Stars. Ann. Astrophys., 27, 813.Google Scholar
53. Morton, D. C. 1964, Theoretical Line Profiles in the Ultraviolet Spectra of Early-Type Stars. Ann. Astrophys., 27, 797.Google Scholar
54. Morton, D. C. 1965, Theoretical Line Profiles in the Ultraviolet Spectra of Early-Type Stars. Astrophys. J., 141, 73.CrossRefGoogle Scholar
55. Orszag, S. A. 1965, Neutron-Star Atmospheres. Astrophys. J., 142, 473.CrossRefGoogle Scholar
56. Osaki, Y. 1966, On the Atmosphere of a Rotating Star. Publ. astr. Soc. Japan, 18, 7.Google Scholar
57. Pagel, B. E. J. 1966, Critical Summary of Abundance Determinations in Stars of Type G and later. Proc. IAU Symposium no. 26, Abundance Determination in Stellar Spectra, p. 272 (Academic Press).Google Scholar
58. Peytremann, E. 1967 (unpublished).Google Scholar
59. Scholz, M. 1967, Eine Analyse des Spektrums des Bo V-Stern τ Scorpii. Z. Astrophys., 65, 1.Google Scholar
60. Sobolev, V. V. 1965, On the Spectra of Hot Stars of Low Luminosity. Trudy astr. Obs. Leningrad. gos. Univ., 22, 3. Google Scholar
61. Conti, P. S., Greenstein, J. L., Spinrad, H., Wallerstein, G., Vardya, M, S. 1967 Astrophys. J., 148, 105.CrossRefGoogle Scholar
62. Strom, S. E., Avrett, E. H. 1966, The Temperature Structure of Early-Type Mode Stellar Atmosphere, II, A Grid of Stellar Models. Astrophys. J. Suppl., 12, 103.Google Scholar
63. Strom, S. E., Kalkofen, W. 1966, The Effect of Departures from LTE on the Stella Continuum Fluxes in the Spectral-Type Range B5-A0. Astrophys, J., 144, 76.CrossRefGoogle Scholar
64. Strom, S. E., Avrett, E. H. 1964, The Temperature Structure of Early-Type Mode Stellar Atmospheres, I. Detailed Analysis of a 10000°K Model. Astrophys. J., 140, 1381 CrossRefGoogle Scholar
65. Swamy, K. S. K. 1966, Profiles of Strong Lines in K-Dwarfs. Astrophys. J., 145, 174 CrossRefGoogle Scholar
66. Terashita, Y., Matsushima, S. 1966, The Structure of White Dwarf Atmospheres. I. Model Atmospheres and Hydrogen-Line Profiles for DA-Type Stars. Astrophys. J. Suppl., 13, 461.CrossRefGoogle Scholar
67. Tsuji, T. 1966, Some Problems on the Atmospheric Structures of Late-Type Stars. Proc. Japan Acad., 42, 258.CrossRefGoogle Scholar
68. Tsuji, T. 1966, The Model Atmospheres of M-Type Stars. Proc. Japan Acad., 42, 7.CrossRefGoogle Scholar
69. Underhill, A. B. 1966, A Critique of Methods based on Complex Representations of Stellar Atmospheres. Proc. IAU Symposium no, 26, p. 118.Google Scholar
70. Underhill, A. B. 1966, Computation of Emergent Flux and Intensities for Blanketing Effect Models and Comparison with Observation. J. quantit. Spectrosc. radiat. Transfer, 6, 675.CrossRefGoogle Scholar
71. Underhill, A. B. The Near Ultraviolet Spectrum from a B Star. Submitted to the J. R. astr. Soc. Can. Google Scholar
72. Unsöld, A. The Chemical Composition of the Stars. Angew. Chemie (International Edition), 3, 481.Google Scholar
73. Vardya, M. S., Kandel, R. On Model Atmospheres for Late-Type Stars. 1967, Ann. Astrophys., 30, 111.Google Scholar
74. Wallerstein, G., Herbig, G. H., Conti, P. S. 1965, Observations of the Lithium Content of Main Sequence Stars in the Hyades. Astrophys. J., 141, 610.CrossRefGoogle Scholar
75. Weidemann, V. 1966, Blanketing in High Gravity Objects. J. quantit. Spectrosc. radiat. Transfer, 6, 691.CrossRefGoogle Scholar
76. Wright, K. O. 1967, Excitation Temperaturea of A and F-Stars. In The Magnetic and Related Stars, Mono Book Corporation, Baltimore (in press).Google Scholar
77. Yamashita, Y. 1965, Curve of Growth Analysis of M-Type Stars. Publ. astr. Soc. Japan, 17. 25.Google Scholar
78. Traving, G. 1966, A Critical Summary of the Results from Early-Type Stars. Proc. IAU Symposium no. 26, p. 213.Google Scholar
79. Wallerstein, G. 1966, Chemical Analysis of Stars of Type Fo–G5. Proc. IAU Symposium no. 26, p. 238.Google Scholar
80. Gebbie, K. B. 1966, Mon. Not. R. astr. Soc. (in press).Google Scholar
81. Guillaume, C. 1965, Theoretical Model of a B 1.5 Star with Line Blanketing. Bull. astr. Inst. Netherl., 18, 175.Google Scholar
1. Ross, J., Aller, L. H. 1967, Astr. J. (in press.)Google Scholar
2. Baschek, B., Holweger, H., Müller, E. A. 1967 (in preparation),Google Scholar
3. Chamaraux, P. 1966, Ann. Astrophys, (in press).Google Scholar
4. Dumont, S. 1966, Profils théoriques des raies de résonances des ioǹs Ca II et Mg II. C. r. Acad, Sci. Paris, 263, 85.Google Scholar
5. Cowley, C. R. 1966, The Abundance of Nickel in the Solar Atmosphere. Astrophys. J., 143, 353.CrossRefGoogle Scholar
6. Fujita, C. 1964, Theoretical Study on Blends of Pairs of Metallic Lines in the Solar Spectrum. Publ. astr. Soc. Japan, 16, 301.Google Scholar
7. Gasson, R. E. M. 1967 (unpublished).Google Scholar
8. Gingerich, O. 1966, Blanketing Approximations for Solar Models. J. quantit. Spectrosc. radiat. Transfer, 6, 609.CrossRefGoogle Scholar
9. Goldberg, L., Kopp, R. A., Dupree, K. 1964, The Abundance of Iron in the Solar Photosphere. Astrophys. J., 140, 707.CrossRefGoogle Scholar
10. Holweger, H. 1967, Ein empirisches Modell der Sonnenatmosphäre mit lokalem thermodynamischen Gleichgewicht. Z. Astrophys., 65, 365.Google Scholar
11. Houtgast, J. 1965, Absolute Intensities in high dispersion solar Bpectra between λ 3000 and λ 4000. K. ned. Akad. Wet. Proc. Sect. Sci., Ser. B., 68, no. 5.Google Scholar
12. de Jager, C. Neven, L. Submitted to Bull. astr. Inst. Netherl. Suppl. Google Scholar
13. de Jager, C. Neven, L. 1967, to be published in Solar Physics, 1. Google Scholar
14. Johnson, H. R. 1964, A Theoretical Study of the Excitation of Sodium in the Solar Photosphere. Ann. Astrophys., 27, 659.Google Scholar
15. King, R. B., Lawrence, G. M., Link, J. K. 1965, Solar Abundances of Gallium, Silver and Indium. Astrophys, J., 142, 386.Google Scholar
16. Kulander, J. L., Jefferies, J. T. 1966, Inference of Velocities from Line Asymetries. Astrophys. J., 146, 194.CrossRefGoogle Scholar
17. O'Mara, B. J. 1967, Line Profiles of Sodium and Calcium in the Sun. Astr. J., in press.Google Scholar
18. Miyamoto, S. Thermal Stability of the Chromosphere and Spicule. Publ. astr. Soc. Japan, 17, 127.Google Scholar
19. Müller, E. A., Mutschlecner, J. P. 1964, Effects of Deviations from LTE on Solar Abundances. Astrophys. J. Suppl., 9, 85.CrossRefGoogle Scholar
19a. Müller, E., Mutschlecner, J. P. 1967 (in press).Google Scholar
20. Müller, E. A. 1967, in Xanthakis, J., Solar Physics, Wiley and Sons.Google Scholar
21. Pagel, B. E. J. 1965, Deductions as to the Accuracy of LTE from Excitation Temperature Measurements, and a Comment on the Abundance of ‘Trace Elements’. Proc. 2nd Harvard-Smithson. Conf. on Stellar Atmospheres, p. 425.Google Scholar
22. Pottasch, S. R. 1964, On the Chemical Composition of the Solar Corona. Mon. Not. R. astr. Soc., 128, 73.CrossRefGoogle Scholar
23. Pottasch, S. R. 1965, On the Determination of the Solar Chemical Composition from a Study of the Ultraviolet Resonance Lines. Ann. Astrophys., 28, 148.Google Scholar
24. Pecker-Wimel, C. Thomas, R. N. 1965, Possible Implications of the Observed Line Profile of (λ 6374) Fe x. Astrophys. J., 141, 834.CrossRefGoogle Scholar
25. Schmahl, G., Schröter, E. H. 1965, Die Li-Häufigkeit und das Isotopenverhältnis Li6/Li7 in Sonnenflecken. Z. Astrophys., 62, 143.Google Scholar
26. Teplitskaya, R. B. 1964, Determination of the Excitation Temperature in the Solar Atmosphere. Astr. Zu., 41, 907.Google Scholar
27. Unno, W. 1966, Influence of Macroturbulence on Chromospheric Doppler Velocities from the Multiplet Method. In The Solar Spectrum(ed. de Jager, C.), p. 120.Google Scholar
28. Wilson, P. R. 1965, On Photospheric Mean Values. Astrophys. J., 142, 1195.CrossRefGoogle Scholar
29. Wilson, P. R. 1966, The Interpretation of Limb Intensity Profiles. Astrophys. J., 146, 241.CrossRefGoogle Scholar
30. Zwaan, C. 1965, Sunspot Models. Rech. astr. Obs. Utrecht, 17, part 4.Google Scholar
31. Czyzak, S. J., Krueger, T. K., Ross, J., Aller, L. H. 1967 (unpublished),Google Scholar
1. Aller, L. H., Ross, J. 1966, Proc. AAS-NASA Symp. Magn. and other Peculiar and Metallic Lune A Stars. Google Scholar
2. Auer, L. H., Mihalas, D., Aller, L. H., Ross, J. E. 1966, The Manganese Star 53 Tauri. II. Fine Analysis. Astrophys. J., 145, 153.CrossRefGoogle Scholar
3. Baschek, B. 1965, Quantitative Analyse des Spektrums des Schnelläufers Wilson 10 367. Z. Astrophys., 61, 27.Google Scholar
4. Böhm-Vitense, E. 1966, Zur Interpretation der Geschwindigkeits- und Intensitäts-variationen der Linien von 2CVn. Z, Astrophys., 64, 326.Google Scholar
5. Böhm-Vitense, E. Line Variations of Stellar Magnetic Fields and the Oblique Rotator Theory. Proceedings of Newcastle Nato Advanced Study Institute on ‘Planetary and Stellar Magnetism’ (in press).Google Scholar
6. Böhm-Vitense, E. On the Spectra of the Magnetic A Stars. Struve Memorial Volume, Editor Hack, H. (in press).Google Scholar
7. Böhm-Vitense, E. 1966, The Crossover Effect in α 2CVn (in preparation).Google Scholar
8. Böhm-Vitense, E. 1966, On the Atmospheres of Helium Stars (in preparation).CrossRefGoogle Scholar
9. Cayrel, R. 1966 (unpublished).Google Scholar
10. Climenhaga, I. L. 1967, The C12/C13 Abundance Ratio in the Red Carbon Stars 19 Piscium, DS Pegasi and Y Canum Venaticorum. Proc. IAU Symp. on Late-Type Stars (in press).Google Scholar
11. Conti, P. S. The Atmospheres of the Metallic-Line Stars in the Hyades. Astrophys. J. Suppl., 11, 95, 1965.CrossRefGoogle Scholar
12. Danziger, I. J. 1965, A High Dispersion Spectral Analysis of the Ba 11 Stars HD 11 6713 and HD 83 548. Mon. Not. R. astr. Soc., 131, 51.CrossRefGoogle Scholar
13. Hardorp, J. 1966, Fine Analysis of the B4P Star 3 Centauri A. Z. Astrophys., 63, 137.Google Scholar
14. Hauck, B. 1967, Thesis, Observatoire de Genève.Google Scholar
15. Hunger, K., van Blerkom, D. A Pure Helium Model Atmosphere. Submitted to Z. Astrophys. Google Scholar
16. Kodaira, K. 1964, Atmosphärenstruktur und chemische Zusammensetzung des Schnelläufers HD 161 817. Z. Astrophys., 59, 139.Google Scholar
17. Mihalas, I., Henshaw, J. L. 1966, Studies of Peculiar A Stars III Model-Atmosphere Line-Strength Calculations with Application to the Ap Stars. Astrophys. J., 144, 25.CrossRefGoogle Scholar
18. Klinglesmith, D. Thesis, Indiana University.Google Scholar
19. Pagel, B. E. J., Powell, A. L. T. 1966, R. Obs. Bull.(in press).Google Scholar
20. Praderie, F. 1965, Sur le spectre infrarouge de quelques étoiles à raies métalliques. C. r. Acad. Sci. Paris, 261, 4625.Google Scholar
21. Searle, L., Lungershausen, W. T., Sargent, W. L. W. 1966, Studies of Peculiar A Stars, IV. The Relative Abundances of Four Iron-peak Elements. Astrophys, J., 145, 141.CrossRefGoogle Scholar
22. Spite, M. 1967, To be published in Ann. Astrophys. Google Scholar
23. Wyller, A. 1966, New C13 Indicators in Stellar Spectra. Astrophys. J., 143, 828.CrossRefGoogle Scholar
24. Wyller, A. 1966 (unpublished).Google Scholar