Hostname: page-component-7bb8b95d7b-qxsvm Total loading time: 0 Render date: 2024-09-18T04:09:22.104Z Has data issue: false hasContentIssue false
  • English
  • Français

Evolutionary Aspects of Circumstellar Matter in Binary Systems

Published online by Cambridge University Press:  14 August 2015

Miroslav Plavec
Miroslav Plavec*
Affiliation:
Dept. of Astronomy, Univ. of California, Los Angeles

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Several groups of close binary stars are considered in an attempt to explain their present state as a consequence of a large-scale mass transfer or mass loss in the past: Algol-like semidetached binaries, some shell stars (AX Mon), some binary X-ray sources (Cen X-3, Her X-1), the recurrent nova T CrB, helium-rich binaries v Sgr and KS Per, and the symbiotic variables.

Algol-like binaries like U Sge cannot be products of a conservative case A of mass transfer; rather, mass loss from system and/or a temporary contact stage must be invoked. Nova T CrB as well as the symbiotic variables probably contain a mass-losing giant and a helium star, which again may be a product of a previous mass transfer of type B. Similarly, some of the X-ray sources may actually be binaries undergoing a second process of mass transfer. The systems v Sgr and KS Per may contain helium stars expanding to the right of the helium main sequence, while the other component may be a rather inactive main-sequence star. Some shell stars may be products of mass transfer. Mass loss from convective envelopes is also discussed.

Loss of mass and of angular momentum from many binary systems must be anticipated. Behavior of the mass-accreting stars may often be decisive for the appearance and evolution of the system.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 51: Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems , 1973 , pp. 216 - 259
Copyright
Copyright © Reidel 1973 

References

Bahcall, J. N. and Bahcall, N. A.: 1972, IAU Circ., No. 2427.Google Scholar
Bath, G. T.: 1969, Astrophys. J. 158, 571.CrossRefGoogle Scholar
Bath, G. T.: 1972, Astrophys. J. 173, 121.Google Scholar
Batten, A. H.: 1967, Publ. Dominion Astroph. Obs. 13, No. 8.Google Scholar
Benson, R. S.: 1970, Bull. Am. Astron. Soc. 2, 295.Google Scholar
Bessell, M. S.: 1972, Astrophys. J. 175, L133.CrossRefGoogle Scholar
Biermann, P. and Kippenhahn, R.: 1971a, Veröffentl. Remeis-Sternw., Bamberg 9, 54.Google Scholar
Biermann, P. and Kippenhahn, R.: 1971b, Astron. Astrophys. 14, 32.Google Scholar
Biermann, P. and Thomas, H. C.: 1971, Veröffentl. Remeis-Sternw., Bamberg 9, 285.Google Scholar
Bolton, C. T.: 1972a, Nature 235, 271.CrossRefGoogle Scholar
Bolton, C. T.: 1972b, IAU Circ., No. 2424.Google Scholar
Boyarchuk, A. A.: 1966, Soviet Astron. 10, 783.Google Scholar
Boyarchuk, A. A.: 1967, Soviet Astron. 11, 8.Google Scholar
Boyarchuk, A. A. 1959, Soviet Astron. 3, 748.Google Scholar
Boyarchuk, A. A.: 1969, in Detre, L. (ed.), Non-Periodic Phenomena in Variable Stars, D. Reidel Publ. Co., p. 395.Google Scholar
Boyarchuk, A. A. and Pronik, I. I.: 1967, Izv. Krymsk. Astrofiz. Obs. 37, 236.Google Scholar
Brucato, R. J. and Kristian, J.: 1972, IAU Circ., No. 2421.Google Scholar
Cester, B. and Pucillo, M.: 1972, preprint.Google Scholar
Cowley, A. P.: 1964, Astrophys. J. 139, 817.Google Scholar
Cowley, A. P.: 1967, Astrophys. J. 147, 609.Google Scholar
Cowley, A. P. and Gugula, E.: 1972, preprint.Google Scholar
Danziger, I. J., Wallerstein, G., and Böhm-Vitense, E.: 1967, Astrophys. J. 150, 239.Google Scholar
Delplace, A. M.: 1970, Astron. Astrophys. 7, 459.Google Scholar
Eggen, O. J., Kron, G. E., and Greenstein, J. L.: 1951, Publ. Astron. Soc. Pacific 62, 171.Google Scholar
Faulkner, J.: 1971, Astrophys. J. 170, L99.Google Scholar
Gaposchkin, S.: 1945, Astron. J. 51, 109.Google Scholar
Hack, M.: 1967, in Hack, M. (ed.), Modern Astrophysics, 163.Google Scholar
Hack, M. and Job, F.: 1965, Z. Astrophys. 62, 203.Google Scholar
Harmanec, P.: 1970a, Bull. Astron. Inst. Czech. 21, 113.Google Scholar
Harmanec, P.: 1970b, Bull. Astron. Inst. Czech. 21, 316.Google Scholar
Harmanec, P., Koubský, P., and Krpata, J.: 1972, Astrophys. Letters 11, 119.Google Scholar
Hazlehurst, J. and Meyer-Hoffmeister, E.: 1971, Veröffentl. Remeis-Sternw., Bamberg 9, 289 Google Scholar
Hickock, J.: 1971, preprint.Google Scholar
Horn, J.: 1971, Bull. Astron. Inst. Czech. 22, 37.Google Scholar
Horn, J., Kříž, S., and Plavec, M.: 1969, Bull. Astron. Inst. Czech. 20, 193.Google Scholar
Horn, J., Kříž, S., and Plavec, M.: 1970, Bull. Astron. Inst. Czech. 21, 45.Google Scholar
Hubbard, W. B., and Wagner, R. L.: 1970, Astrophys. J. 159, 93.Google Scholar
Hutchings, J. B. and Redman, R. O.: 1972, Publ. Astron. Soc. Pacific 84, 240.Google Scholar
Hynek, A. J.: 1940, Contr. Perkins Obs., No. 14.Google Scholar
Iben, I.: 1967, Ann. Rev. Astron. Astrophys. 5, 571.Google Scholar
Kippenhahn, R. and Weigert, A.: 1967, Z. Astrophys. 65, 251.Google Scholar
Kippenhahn, R., Kohl, K., and Weigert, A.: 1967, Z. Astrophys. 66, 58.Google Scholar
Kopal, Z.: 1955, Ann. Astrophys. 18, 379.Google Scholar
Kopal, Z.: 1971, Publ. Astron. Soc. Pacific 83, 521.Google Scholar
Kopal, Z. and Shapley, M. B.: 1956, Jodrell Bank Ann. 1, 141.Google Scholar
Kraft, R. P.: 1958, Astrophys. J. 127, 625.CrossRefGoogle Scholar
Kraft, R. P.: 1972, Contr. Lick Obs., No. 368.Google Scholar
Kříž, S.: 1969a, Bull. Astron. Inst. Czech. 20, 127.Google Scholar
Kříž, S.: 1969b, in Hack, M. (ed.), Mass Loss from Stars, D. Reidel Publ. Co., p. 257.CrossRefGoogle Scholar
Kruszewski, A.: 1966, Adv. Astron. Astrophys. 4, 233.Google Scholar
Lamb, D. Q. and Sorvari, J. M.: 1972, IAU Circ. No. 2422.Google Scholar
Lauterborn, D.: 1970, Astron. Astrophys. 7, 150.Google Scholar
Lauterborn, D. and Weigert, A.: 1972, Astron. Astrophys. 18, 294.Google Scholar
Liller, W.: 1972, IAU Circ., No. 2415.Google Scholar
McCluskey, G. E. and Kondo, Y.: 1972, preprint.Google Scholar
Moss, D. L.: 1971, Monthly Notices Roy. Astron. Soc. 153, 41.Google Scholar
Nariai, K.: 1963, Publ. Astron. Soc. Japan 15, 7.Google Scholar
Nariai, K.: 1967, Publ. Astron. Soc. Japan 19, 564.Google Scholar
Paczyński, B.: 1965, Acta Astron. 15, 89.Google Scholar
Paczyński, B.: 1956b, Acta Astron. 15, 197.Google Scholar
Paczyński, B.: 1970, Acta Astron. 20, 47.Google Scholar
Paczyński, B.: 1971a, Ann. Rev. Astron. Astrophys. 9, 183.Google Scholar
Paczyński, B.: 1971b, Acta Astron. 21, 1.Google Scholar
Paczyński, B. and Ziółkowski, J.: 1967, Acta Astron. 17, 7.Google Scholar
Paczyński, B., Ziółkowski, J., and żytkow, A.: 1969, in Hack, M. (ed.), Mass Loss from Stars, D. Reidel Publ. Co., p. 237.CrossRefGoogle Scholar
Paczyński, B. and Sienkiewicz, R.: 1972, preprint.Google Scholar
Peters, G. J.: 1972, Publ. Astron. Soc. Pacific 84, 334.Google Scholar
Péton, A.: 1971, Compt. Rend. Acad. Sci. Paris, B 273, 1062.Google Scholar
Prendergast, K. H. and Burbidge, G. J.: 1968, Astrophys. J. 151, L83.Google Scholar
Plavec, M.: 1964, Bull. Astron. Inst. Czech. 15, 156.Google Scholar
Plavec, M.: 1967, Bull. Astron. Inst. Czech. 18, 334.Google Scholar
Plavec, M.: 1968, Adv. Astron. Astrophys. 6, 201.Google Scholar
Plavec, M.: 1970a, Publ. Astron. Soc. Pacific 82, 957.Google Scholar
Plavec, M.: 1970b, in Slettebak, A. (ed.), Stellar Rotation, D. Reidel Publ. Co., p. 133.Google Scholar
Plavec, M. and Horn, J.: 1969, in Hack, M. (ed.), Mass Loss from Stars, D. Reidel Publ. Co., p. 242.Google Scholar
Plavec, M., Kříž, S., and Horn, J.: 1969, Bull. Astron. Inst. Czech. 20, 41.Google Scholar
Popper, D. M.: 1970, in Gyldenkerne, K. and West, R. (eds.), Mass Loss and Evolution in Close Binaries, p. 20.Google Scholar
Refsdal, S. and Weigert, A.: 1969, Astron. Astrophys. 1, 167.Google Scholar
Sahade, J., (ed.): 1962, Symposium on Stellar Evolution, La Plata, p. 225.Google Scholar
Sahade, J.: 1971, Veröffentl. Remeis-Sternw. Bamberg 9, 285.Google Scholar
Sato, K.: 1971, Publ. Astron. Soc. Japan 23, 335.Google Scholar
Schmidt, H.: 1959, Z. Astrophys. 48, 249.Google Scholar
Schreier, E., Levinson, R., Gursky, H., Kellogg, E., Tananbaum, H., and Giacconi, R.: 1972, Astrophys. J. 172, L79.Google Scholar
Seydel, F. L.: 1929, Publ. Am. Astron. Soc. 6, 278.Google Scholar
Struve, O.: 1946, Astrophys. J. 104, 253.Google Scholar
Struve, O. and Huang, S.-S.: 1958, in Flügge, S. (ed.), Handbuch der Physik, Springer Verlag, 50, p. 269.Google Scholar
Svechnikov, M. A.: 1955, Peremennyje Zvezdy 10, 252.Google Scholar
Tananbaum, H., Gursky, H., Kellogg, E. M., Levinson, R., Schreier, E., and Giacconi, R.: 1972, Astrophys. J. 174, L143.Google Scholar
Underhill, A. B.: 1952, Publ. Dominion Astrophys. Obs. 9, 129.Google Scholar
Underhill, A. B.: 1966, Early-Type Stars, D. Reidel Publ. Co., p. 233.Google Scholar
Van den Heuvel, E. P. J.: 1970, in Slettebak, A. (ed.), Stellar Rotation, D. Reidel Publ. Co., p. 178.Google Scholar
Van den Heuvel, E. P. J. and Heise, J.: 1972, Nature Phys. Sci. 239, 67.Google Scholar
Walker, M. F.: 1953, Astrophys. J. 118, 481.Google Scholar
Wallerstein, G., Greene, T. F., and Tomley, L. J.: 1967, Astrophys. J. 245, 150.Google Scholar
Webster, B. L. and Murdin, P.: 1972, Nature 235, 37.Google Scholar
Weigert, A.: 1968, in Perek, L. (ed.), Highlights of Astronomy, D. Reidel Publ. Co. p. 414.Google Scholar
Widing, K. G.: 1966, Astrophys. J. 143, 121.Google Scholar
Wilson, R. E.: 1972, preprint.Google Scholar
Wright, K. O.: 1957, Publ. Astron. Soc. Pacific 69, 552.Google Scholar
Ziółkowski, J.: 1969, Astrophys. Space Sci. 3, 14.Google Scholar
Ziółkowski, J.: 1970, Acta Astron. 20, 213.Google Scholar