Skip to main content Accessibility help
×
Hostname: page-component-84b7d79bbc-4hvwz Total loading time: 0 Render date: 2024-07-30T09:18:29.306Z Has data issue: false hasContentIssue false

References

Published online by Cambridge University Press:  05 December 2011

Richard Dodd
Affiliation:
Victoria University of Wellington
Get access

Summary

Image of the first page of this content. For PDF version, please use the ‘Save PDF’ preceeding this image.'
Type
Chapter
Information
Publisher: Cambridge University Press
Print publication year: 2011

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Abdo, A. A., Ackermann, M., Ajello, M.et al. (2009). Discovery of pulsations from the pulsar J0205+6449 in SNR 3C 58 with the FERMI γ-ray space telescopeApJL, 699, L102–L107.CrossRefGoogle Scholar
Abdo, A. A., Ackermann, M., Ajello, M.et al. (2010). The first catalog of active galactic nuclei detected by the FERMI Large Area Telescope. ApJ, 715, 429–457.CrossRefGoogle Scholar
Abramowitz, M. & Stegun, I. A. eds (1972). Handbook of Mathematical Functions. New York: Dover Publications Inc., p. 67.Google Scholar
Albacete-Colombo, J. F., Damiani, F., Micela, G., Sciortino, S. & Harnden, F. R., Jr. (2008). An X-ray survey of low-mass stars in Trumpler 16 with CHANDRA. A&A, 490, 1055–1070.Google Scholar
Alexeev, I. I., Belenkaya, E. S., Slavin, J. A.et al. (2010). Mercury's magnetospheric magnetic field after the first two MESSENGER flybys. Icarus, 209, 23–39.CrossRefGoogle Scholar
Alder, K. (2004). The Measure of All Things. London: Abacus.Google Scholar
Allen, C. W. (1951). Dex. Observatory, 71, 157.Google Scholar
Allen, R. H. (1899). Star Names and their Meanings. New York: G. E. Stechert & Co.Google Scholar
Aller, L. H. (1963). Astrophysics: The Atmospheres of the Sun and Stars, 2nd edn. New York: The Roland Press Company.Google Scholar
Alonso-Medina, A., Colón, C., Montero, J. L. & Nation, L. (2009). Stark broadening of PbIV spectral lines of astrophysical interest. MNRAS, 401, 1080–1090.CrossRefGoogle Scholar
Amari, S., Hoppe, P., Zinner, E. & Lewis, R. S. (1992). Interstellar SiC with unusual isotopic compositions: Grains from a supernova? ApJ, 394, L43–L46.CrossRefGoogle Scholar
Anderson, B. J., Acuña, M. H., Korth, H.et al. (2010). The magnetic field of Mercury. Space Sci. Rev., 152, 307–339.CrossRefGoogle Scholar
Astronomical Almanac for 1995, The (1994). London: HMSO.
Atkin, K. (2007). Size matters. A&G, 48, 4.7.Google Scholar
Atwood, W. B.Abdo, A. A., Ackermann, M.et al. (2009). The Large Area Telescope on the FERMI γ-ray space telescope mission. ApJ, 697, 1071–1102.CrossRefGoogle Scholar
Bagnulo, S., Szeifert, T., Wade, G. A., Landstreet, J. D. & Mathys, G. (2002). Measuring magnetic fields of early type stars with FORS1 at the VLT. A&A, 389, 191–201.Google Scholar
Barlow, C. W. C. & Bryan, G. H. (1956). Elementary Mathematical Astronomy. London: University Tutorial Press Ltd., p. 125.Google Scholar
Battat, J. B. R., Murphy, T. W., Jr., Adelberger, E. G.et al. (2009). The Apache Point Lunarranging Operation (APOLLO): Two years of millimeter-precision measurements of the Earth–Moon range. PASP, 121, 29–40.CrossRefGoogle Scholar
de la Beaujardière, J.-F., Canfield, R. C. & Leka, K. D. (1993). The morphology of flare phenomena, magnetic fields and electric currents in active regions. III NOAA active region 6233 (1990 August). ApJ, 411, 378–382.CrossRefGoogle Scholar
Bedding, T. R., Butler, R. P., Carrier, F.et al. (2006). Solar-like oscillations in the metalpoor subgiant v Indi: constraining the mass and age using asteroseismology. ApJ, 647, 558–563.CrossRefGoogle Scholar
Beech, M. (2008). The reluctant parsec and the overlooked light-year. Observatory, 128, 489–494.Google Scholar
Bemporad, A. & Mancusco, S. (2010). First complete determination of plasma physical parameters across a coronal mass ejection driven shock. ApJ, 720, 130–143.CrossRefGoogle Scholar
Bessel, F. W. (1838). On the parallax of 61 Cygni. MNRAS, 4, 152–161.Google Scholar
Bessell, M. S. (1992). In The Astronomy and Astrophysics Encyclopedia, ed. S. P., Maran. Cambridge: Cambridge University Press, p. 403.Google Scholar
Bessell, M. S. (2001). In Encyclopedia of Astronomy & Astrophysics, Vol. 2, ed. P., Murdin, Bristol: IoP, pp. 1638–1644.Google Scholar
,BIPM (2006). The International System of Units, 8th edn. France: CIPM.Google Scholar
Blanco, V. M. & McCuskey, S. W. (1961). Basic Physics of the Solar System. Reading, MA: Addison-Wesley Publishing Company, Inc.Google Scholar
Blauuw, A., Gum, C. S., Pawsey, J. L. & Westerhout, G. (1960). The new IAU system of galactic coordinates (1958 revision). MNRAS, 121, 123–131.CrossRefGoogle Scholar
Bleaney, B. I. & Bleaney, B. (1962). Electricity and Magnetism. Oxford: Clarendon Press.Google Scholar
Bohlin, R. C. & Gilliland, R. L. (2004). Hubble SpaceTelescope absolute spectrophotometry from the far ultraviolet to the infrared. AJ, 127, 3508–3515.CrossRefGoogle Scholar
Bok, B. J. (1937). The Distribution of the Stars in Space. Chicago, IL: The University of Chicago Press.Google Scholar
Bradley, P. A. (1993). Methods of asteroseismology for white dwarf stars. Baltic Astr., 2, 545–558.Google Scholar
Brimblecombe, S., Gallannaugh, D. & Thompson, C., eds. (1998). The Hutchinson Encyclopedia of Science. Oxford: HeliconGoogle Scholar
Brown, M. E. & Schaller, E. L. (2007). The mass of the dwarf planet Eris. Science, 316, 1585.CrossRefGoogle ScholarPubMed
Browning, D. R., ed. (1969). Spectroscopy. London: McGraw-Hill.Google Scholar
Burke, B. F. & Graham-Smith, F. (2002). An Introduction to Radio Astronomy. 2nd edn. Cambridge: Cambridge University Press.Google Scholar
Burningham, B., Pinfield, D. J., Leggett, S. K.et al. (2008). Exploring the substellar temperature region down to ∼500 K. MNRAS, 391, 320–333.CrossRefGoogle Scholar
Cairns, W. (2007). About the Size of It. London: MacMillan.Google Scholar
Capitaine, N. & Guinot, B. (2008). The astronomical units. arXiv:0812.2970v1 [astro-ph].
Cardarelli, F. (2003). Encyclopedia of Scientific Units, Weights and Measures. London: Springer.CrossRefGoogle Scholar
Chambers, G. F. (1889). Astronomy. I: The Sun, Planets and Comets. Oxford: Clarendon Press.Google Scholar
Chang, R. (2005). Chemistry, 8th edn. New York: McGraw-Hill.Google ScholarPubMed
Cohen, M., Walker, R. G., Barlow, M. J. & Deacon, J. R. (1992). Spectral irradiance calibration in the infrared. I. Ground-based and IRAS broadband calibrations. AJ, 104, 1650–1657.CrossRefGoogle Scholar
Cohen, M., Wheaton, W. A. & Megeath, S. T. (2003). Spectral irradiance calibration in the infrared XIV: The absolute calibration of 2MASS. AJ, 126, 1090–1096.CrossRefGoogle Scholar
Collins, II, G. W. (1989). The Fundamentals of Stellar Astrophysics. New York: W. H. Freeman and Company.Google Scholar
Coulson, C. A. & Boyd, T. J. M. (1979). Electricity. London: Longman.Google Scholar
Cowley, C. R. (1995). An Introduction to Cosmochemistry. Cambridge: Cambridge University Press.CrossRefGoogle Scholar
Cox, A. N. (2000). Allen's Astrophysical Quantities, 4th edn, ed. A. N., Cox. New York: Springer.Google Scholar
Culhane, J. L. & Sanford, P. W. (1981). X-ray Astronomy. London: Faber & Faber.Google Scholar
Dodd, R. J. (2004). Data mining in the young open cluster IC2391. MNRAS, 355, 959–973.CrossRefGoogle Scholar
Dodd, R. J. (2007). Unified absolute spectrophotometry for star clusters, ed. C., Sterken. ASP Conference Series, 364, pp. 237–254.Google Scholar
Duffard, R., Ortiz, J. L., Santos Sanz, P.et al. (2008). A study of the photometric variations on the dwarf planet (136199) Eris. A&A, 479, 877–881.Google Scholar
Dyson, F. W. (1913). Report of the Royal Astronomical Society meeting on 14 March 1913. Observatory, 36, 160.Google Scholar
Dyudina, U. A., del Genio, A. D., Ingersoll, A. P.et al. (2004). Lightning on Jupiter observed in the Hα line by the Cassini imaging science subsystem. Icarus, 172, 24–36.CrossRefGoogle Scholar
Emerich, C., Lamarre, J. M., Gispert, R.et al. (1988). Temperature of the nucleus of comet Halley. ESA Proceedings of International Symposium on the Diversity and Similarity of Comets, pp. 703–706.Google Scholar
Evans, D. S. (1954). Teach Yourself Astronomy. London: English Universities Press Ltd.Google Scholar
Evensen, K. M., Wells, J. S., Petersen, F. R.et al. (1972). Speed of light from direct frequency and wavelength measurements of the methane-stabilized laser. PRL, 29, 1346–1349.CrossRefGoogle Scholar
Ferdman, R. D., Stairs, I. H., Kramer, M.et al. (2010). The precise mass measurement of the intermediate-mass binary pulsar PSR J1802–2124. ApJ, 711, 764–771.CrossRefGoogle Scholar
Ferriere, K. (2001). The interstellar environment of our galaxy. Rev. Mod. Phys., 73, 1031–1066.CrossRefGoogle Scholar
Fixler, J. B., Foster, G. T., McGuirk, J. M. & Kasevich, M. A. (2007). Atom interferometer measurement of the Newtonian constant of gravity. Science, 315, 74–77.CrossRefGoogle Scholar
Flasar, F. M., Achterberg, R. K., Conrath, B. J.et al. (2005). Titan's atmospheric temperatures, winds and composition. Science, 308, 975–978.CrossRefGoogle ScholarPubMed
Fouqué, P., Chevallier, L., Cohen, M.et al. (2000). An absolute calibration of DENIS. A&AS, 141, 313–317.Google Scholar
Funk, I. K., Thomas, C., Vizetelly, F. M. & Funk, C. E. eds. (1946). Funk & Wagnalls New Standard Dictionary of the English Language, Vols I and II. London: The Waverley Book Company Ltd.Google Scholar
Gezari, D. Y., Schmitz, M., Pitts, P. S. & Mead, J. M. (1993). Catalog of Infrared Observations, 3rd edn. Greenbelt, MD: NASA reference publication, p. 1294.Google Scholar
Girard, G. (1994). The third periodic verification of national prototypes of the kilogram (1988–1992). Metrologia, 31, 317–336.CrossRefGoogle Scholar
Gnedin, Y. N. (1997). Chromospheres, activity and magnetic fields. In Fundamental Stellar Properties: The Interaction Between Observation and Theory, ed. T. R., Beddinget al.Dordrecht: Kluwer, pp. 245–252.CrossRefGoogle Scholar
Gould, A., Udalski, A., Monard, B.et al. (2009). The extreme microlensing event OGLE-2007-BLG-224: Terrestrial parallax of a thick-disk brown dwarf. ApJL, 698, 147–151.CrossRefGoogle Scholar
Hansen, C. J., Kawaler, S. D. & Trimble, V. (2004). Stellar Interiors: Physical Principles, Structure and Evolution. New York: Springer-Verlag.CrossRefGoogle Scholar
Harris, III, D. L., Strand, K. Aa. & Worley, C. E. (1963). Empirical data on stellar masses, luminosities and radii. In Basic Astronomical Data, ed. K. Aa., Strand. Chicago IL: University of Chicago Press, pp. 273–292.Google Scholar
Hawkins, J. M. & Allen, R. eds. (1991). The Oxford Encyclopedic English Dictionary. Oxford: Clarendon Press.Google Scholar
Hearnshaw, J. B. (1986). The Analysis of Starlight. Cambridge: Cambridge University Press.Google Scholar
Hearnshaw, J. B. (1996). The Measurement of Starlight: Two Centuries of Astronomical Photometry. Cambridge: Cambridge University Press.Google Scholar
Henriksen, M. J. & Tittley, E. R. (2002). CHANDRA observations of the A3266 galaxy cluster merger. ApJ, 577, 701–709.CrossRefGoogle Scholar
Herbst, E. (2001). In Encyclopedia of Astronomy & Astrophysics, Vol. 2, ed. P., Murdin, Bristol: IoP. pp. 1258–1266.Google Scholar
Hohle, M. M.Eisenbeiss, T., Mugrauer, M.et al. (2009). Photometric study of the OB star clusters NGC1502 and NGC2169 and mass estimation of their members at the University Observatory Jena. AN, 330, 511.Google Scholar
Holland, W. S., Greaves, J. S., Zuckerman, B.et al. (1998). Submillimeter images of dusty debris around nearby stars. Nature, 392, 788–791.CrossRefGoogle Scholar
Hollis, J. M., Chin, G. & Brown, R. L. (1985). An attempt to detect mass loss from α Lyrae with the VLA. ApJ, 294, 646–648.CrossRefGoogle Scholar
Hovestadt, D., Hilchenbach, M., Bürgi, A.et al. (1995). CELIAS: Charge, Element and Isotope Analysis System for SOHO. Sol. Phys., 162, 441–481.CrossRefGoogle Scholar
Huang, T.-Y., Han, C.-H., Yi, Z.-H., & Xu, B.-X. (1995). What is the astronomical unit of length? A&A, 298, 629–633.Google Scholar
Hubble, E. P. (1926). Extragalactic nebulae. ApJ, 64, 321–369.CrossRefGoogle Scholar
Hubble, E. P. (1929). A relation between distance and radial velocity among extra-galactic nebulae. PNAS, 15, 168–173.CrossRefGoogle ScholarPubMed
Irwin, J. A. (2007). Astrophysics: Decoding the Cosmos. Chichester: John Wiley & Sons Ltd.Google Scholar
Józsa, G. I. G., Garrett, M. A., Oosterloo, T. A.et al. (2009). Revealing Hanny's Voorwerp: radio observations of IC2497. A&A, 500, L33–L36.Google Scholar
Karovska, M. & Sasselov, D. (2001). In Encyclopedia of Astronomy & Astrophysics, vol. 4, ed. P., Murdin. Bristol: IoP, pp. 3068.Google Scholar
Kaye, G. W. C. & Laby, T. H. (1959). Tables of Physical and Chemical Constants and some Mathematical Functions, 12th edn. London: Longmans, Green and Co.Google Scholar
Keenan, P. C. (1963). Classification of stellar spectra. In Basic Astronomical Data, ed. K. Aa., Strand. Chicago: University of Chicago Press, pp. 78–122.Google Scholar
King, H. C. (1955). The History of the Telescope. London: Charles Griffin & Co. Ltd.Google Scholar
Kirkpatrick, J. D. (2005). New spectral types L and T. ARA&A., 43, 195–246.CrossRefGoogle Scholar
Klioner, S. A. (2007). Relativistic scaling of astronomical quantities and the system of astronomical units. A&A, 478, 951–958.Google Scholar
Korhonen, H., Hubrig, S., Berdyugina, S. V.et al. (2009). First measurement of the magnetic field on FK Com and its relation to the contemporaneous star-spot locations. MNRAS, 395, 282–289.CrossRefGoogle Scholar
Kurucz, R. L. (1979). Model atmospheres for G, F, A, B and O stars. ApJS, 40, 1–340.CrossRefGoogle Scholar
Kutner, M. L. (2003). Astronomy: A Physical Perspective, 2nd edn. Cambridge: Cambridge University Press.CrossRefGoogle Scholar
Landstree, J. D. (2001). In Encyclopedia of Astronomy & Astrophysics, vol. 2, ed. P., Murdin. Bristol: IoP, pp. 1508–1514.Google Scholar
Lang, K. R. (2006). Astrophysical Formulae. Vols I and II: Berlin: Springer-Verlag.CrossRefGoogle Scholar
Leggett, S. K., Cushing, M. C., Saumon, D.et al. (2009). The physical properties of four 600K T dwarfs. ApJ, 695, 1517–1526.CrossRefGoogle Scholar
Leschiutta, S. (2001). In Encyclopedia of Astronomy & Astrophysics, vol. 4, ed. P., Murdin. Bristol: IoP, pp. 3313–3315.Google Scholar
Liddell, H. G. & Scott, R. (1996). A Greek – English Lexicon. Oxford: Clarendon Press.Google Scholar
Lignières, F., Petit, P., Böhm, T. & Aurière, M. (2009). First evidence of a magnetic field on Vega. A&A, 500, L41–L44.Google Scholar
Longair, M. S. (1989). Royal Observatory Edinburgh: Research and Facilities Handbook. Edinburgh: ROE, p. 79.Google Scholar
Love, S. G. & Brownlee, D. E. (1993). Adirect measurement of the terrestrial accretion rate of cosmic dust. Science, 262, 550–553.CrossRefGoogle Scholar
Lovell, B. & Clegg, J. A. (1952). Radio Astronomy. London: Chapman & Hall Ltd.Google Scholar
Lucas, P. W., Tinney, C. G., Burningham, B.et al. (2010). Discovery of a very cool brown dwarf amonst the ten nearest stars to the Solar System. arXiv:1004.0317v1[astroph. SR].
Lyne, A. G., Pritchard, R. S. & Graham-Smith, F. (1993). 23 years of Crab pulsar rotational history. MNRAS, 265, 1003–1012.CrossRefGoogle Scholar
McCarthy, D. D. & Petit, G. (2003). IERS Technical Note, 32. IERS Conventions (2003). Frankfurt am Main: Verlag des Bundesamtes für Kartographie und Geodäsie.Google Scholar
Manchester, R. N., Hobbs, G. B., Teoh, A. & Hobbs, M. (2005). The Australia Telescope National Facility pulsar catalogue. AJ, 129, 1993–2006CrossRefGoogle Scholar
Mather, J. C., Cheng, E. S., Cottingham, D. A.et al. (1994). Measurement of the cosmic microwave background spectrum by the COBEFIRAS instrument. ApJ, 420, 439–444.CrossRefGoogle Scholar
Mayes, V. (1994). Unit prefixes for use in astronomy. QJRAS, 35, 569–572.Google Scholar
Menzel, D. H. (1960). Fundamental Formulas of Physics. Vols 1 and 2. New York: Dover Publications Inc.Google Scholar
Mills, I., Cvitaš, T., Homann, K., Kallay, N. & Kuchitsu, K. (1993). Quantities, Units and Symbols in Physical Chemistry, 2nd edn. International Union of Pure and Applied Chemistry. Oxford: Blackwell Science.Google Scholar
Mills, I. M., Mohr, P. J., Quinn, T. J., Taylor, B. N. & Williams, E. R. (2005). Redefinition of the kilogram: a decision whose time has come. Metrologia, 42, 71–80.CrossRefGoogle Scholar
Miura, T., Arakida, H., Kasai, M. & Kuramata, S. (2009). Secular increase of the astronomical unit: a possible explanation in terms of the total angular-momentum conservation law. PASJ, 61, 1247–1250.CrossRefGoogle Scholar
Moffatt, J. (1950). A New Translation of the Bible. London: Hodder and Stoughton Ltd.Google Scholar
Mohr, P. J., Taylor, B. N.&Newell, D. B. (2007). The fundamental physical constants. Phys. Today, 60(7), 52–55.CrossRefGoogle Scholar
Monet, D. G., Levine, S. E., Canzian, B.et al. (2003). The USNO-B Catalog. AJ, 125, 984–993.CrossRefGoogle Scholar
Moore, C. E. (1959). A Multiplet Table of Astrophysical Interest. Washington, DC: US Department of Commerce.Google Scholar
Moore, P. A. (2001). In Encyclopedia of Astronomy & Astrophysics, vol. 1, ed. P., Murdin. Bristol: IoP, p. 464.Google Scholar
Muhleman, D. O., Holdridge, D. B. & Block, N. (1962). The astronomical unit determined by radar reflections from Venus. AJ, 67, 191–203.CrossRefGoogle Scholar
Murray, C. A. (1989). The transformation of coordinates between the systems of B1950.0 and J2000.0, and the principal galactic axes referred to J2000.0. A&A, 218, 325–329.Google Scholar
Noerdlinger, P. D. (2008). Solar mass loss, the astronomical unit, and the scale of the Solar System. 2008arXiv0801.3807N, 1–31.
Pannekoek, A. (1961). A History of Astronomy. London: George Allen & Unwin Ltd.Google Scholar
Patilla, P. (2000). Measuring Up Size. London: Belitha Press Ltd.Google Scholar
Pease, D. O., Drake, J. J. & Kashyap, V. L. (2006). The darkest bright star: CHANDRA X-ray observations of Vega. ApJ, 636, 426–431.CrossRefGoogle Scholar
Penzias, A. A. & Wilson, R. W. (1965). A measurement of excess antenna temperature at 4080 Mc/s. ApJ, 142, 419–421.CrossRefGoogle Scholar
Perryman, M. A. C., Lindegren, L., Kovalevsky, J.et al. (1997). The Hipparcos Catalogue. A&A, 323, L49–L52.Google Scholar
Pitjeva, E. V. (2005). High-precision ephemerides of planets – EPM and determination of some astronomical constants. Solar System Res., 39, 176–186.CrossRefGoogle Scholar
Pitjeva, E. V. & Standish, E. M. (2009). Proposals for the masses of the three largest asteroids, the Earth – Moon mass ratio and the astronomical unit, Celest. Mech. Dyn. Astr., 103, 365–372.CrossRefGoogle Scholar
Reddish, V. C. (1978). Stellar Formation. Oxford: Pergamon Press.Google Scholar
Ridpath, I. (2007). Oxford Dictionary of Astronomy, 2nd edn. Oxford: Oxford University Press.Google Scholar
Rufener, F. & Nicolet, B. (1988). A new determination of the Geneva photometric passbands and their absolute calibration. A&A, 206, 357–374.Google Scholar
Rutherford, E. (1929). Origin of actinium and age of the Earth. Nature, 123, 313–314.CrossRefGoogle Scholar
Sackman, I.-J., Boothroyd, A. I. & Kraemer, K. E. (1993). Our Sun. III: Present and future. ApJ, 418, 457–468.CrossRefGoogle Scholar
Saha, M. N. (1921). On the physical theory of stellar spectra. Proc. Roy. Soc. London, A99, 135–138.CrossRefGoogle Scholar
Sandage, A. (1961). The Hubble Atlas of Galaxies. Publications of the Carnegie Institution of Washington No. 618, Washington.Google Scholar
Schramm, D. N. (1990). The Age of the Universe: Concordance. In Astrophysical Ages and Dating Methods, ed. E., Vangioni–Flam, et al. Gif-sur-Yvette, France: Editions Frontières, pp. 365–383.Google Scholar
Shane, C. D. & Wirtanen, C. A. (1954). The distribution of the extragalactic nebulae. AJ, 59, 285–306.CrossRefGoogle Scholar
Shklovskii, I. S. (1970). Possible causes of the scalar increase in pulsar periods. Sov. Astr., 13, 562–565.Google Scholar
Sidgwick, J. B. (1955). Observational Astronomy for Amateurs. London: Faber & Faber Ltd.Google Scholar
Spencer-Jones, H. (1956). General Astronomy. London: Edward Arnold (Publishers) Ltd.Google Scholar
Stencel, R. E.Creech-Eakman, M., Hart, A.et al. (2008). Interferometric studies of the extreme binary ε Aurigae: pre-eclipse observations. ApJL, 689, L137–L140.CrossRefGoogle Scholar
Sterken, C. & Manfroid, J. (1992). Astronomical Photometry: A Guide. Dordrecht: Kluwer Academic Publishers.CrossRefGoogle Scholar
Straižys, V. (1992). Multicolor Stellar Photometry. Tucson, AZ: Pachart Publishing House.Google Scholar
Struve, O., Lynds, B. & Pillans, H. (1959). Elementary Astronomy. New York: Oxford University Press.Google Scholar
Sumi, T., Udalski, A., Szymański, M.et al. (2004). The Optical Gravitational Lensing Experiment: catalogue of stellar proper motions in the OGLE II Galactic bulge fields. MNRAS, 348, 1439–1450.CrossRefGoogle Scholar
Taylor, J. H., Manchester, R. N. & Lyne, A. G. (1993). Catalog of 558 pulsars. ApJS, 88, 529–568.CrossRefGoogle Scholar
Thompson, G. I., Nandy, K., Jamar, C.et al. (1978). Catalogue of Stellar Ultraviolet Fluxes. London: Science Research Council.Google Scholar
Thorsett, S. E. (2001). In Encyclopedia of Astronomy & Astrophysics, vol. 3, ed. P., Murdin. Bristol: IoP, pp. 2177–2183.Google Scholar
Trimble, V. (2010). A review of An Introduction to the Theory of Stellar Structure and Evolution, 2nd edn. Observatory, 130, 185–186.Google Scholar
Trumpler, R. J. (1930). Lick Observatory Bulletin, No. 420.
Urry, C. M. (1988). X-ray timing of active galactic nuclei. Lecture Notes in Physics, 307, 257–274.CrossRefGoogle Scholar
van Biesbroeck, G. (1963). Star catalogues and charts. In Basic Astronomical Data, ed. K., Aa. Strand. Chicago IL: University of Chicago Press, pp. 471–480.Google Scholar
van Duinen, R. J., Aalders, J. W. G., Wesselius, P. R.et al. (1975). The ultraviolet experiment onboard the Astronomical Netherlands Satellite –ANS. A&A, 39, 159–163.Google Scholar
van Leeuwen, F. (2007). Hipparcos, the New Reduction of the Raw Data. London: Springer.
Verbiest, J. P. W., Lorimer, D. R. & McLaughlin, M. A. (2010). Lutz – Kelker bias in pulsar parallax measurements. MNRAS, 405, 564–572.Google Scholar
Viala, Y. P. (1986). Chemical equilibrium from diffuse to dense interstellar clouds. I: Galactic molecular clouds. A&AS, 64, 391–437.Google Scholar
Wall, J. V. & Jenkins, C. R. (2003). Practical Statistics for Astronomers. Cambridge: Cambridge University Press.CrossRefGoogle Scholar
Weaver, T. A., Zimmerman, G. B. & Woosley, S. E. (1978). Pre-supernova evolution of massive stars. ApJ, 225, 1021–1029.CrossRefGoogle Scholar
Weisberg, J. M., Cordes, J. M., Kuan, B.et al. (2004). Arecibo 430 MHz pulsar polarimetry: Faraday rotation measures and morphological classifications. ApJS, 150, 317–341.CrossRefGoogle Scholar
Wesselius, P. R., van Duinen, R. J., Aalders, J. W. G. & Kester, D. (1980). Ultraviolet colours of main-sequence stars. A&A, 85, 221–232.Google Scholar
Wesselius, P. R., van Duinen, R. J., de Jong, A. R. W.et al. (1982). ANS ultraviolet photometry, catalogue of point sources. A&AS, 49, 427–474.Google Scholar
Weygand, J. M., Ipavich, F. M., Wurz, P.Paquette, J. A. & Bochsler, P. (1999). Plasma dynamics and diagnostics in the solar transition region and corona: Determination of the argon isotope ratio of the solar wind using SOHO/CELIAS/MTOF. Proceedings of 8th SOHOWorkshop, ESA SP-446, pp. 701–705.
White, V., ed (2008). British Astronomical Association, London: BAA. Handbook for 2008.Google Scholar
Wieser, M. E. & Berglund, (2009). Atomic weights of the elements 2007 (IUPAC technical report). Pure Appl. Chem., 81, 2131–2156.CrossRefGoogle Scholar
Wilkins, G. A. (1989). IAU Style Manual, Comm. 5. In IAU Transactions, XXB.
Winget, D. E., Nather, R. E., Clemens, J. C.et al. (1994). Whole Earth Telescope observations of the DBV white dwarf GD358. ApJ, 430, 839–849.CrossRefGoogle Scholar
Wolfe, A. M., Jorgenson, R. A., Robishaw, T., Heiles, C. & Prochaska, J. A. (2008). An 84 μG magnetic field in a galaxy at redshift z = 0.692. Nature, 455, 638–640.CrossRefGoogle Scholar
Wollard, E. W. & Clemence, G. M. (1966). Spherical Astronomy. New York and London: Academic Press.Google Scholar
Wright, E. L. (2006). A cosmology calculator for the World Wide Web. PASP, 118, 1711–1715.CrossRefGoogle Scholar
Yang, Y.-G. (2009). BVR observations and period variation of the neglected contact binary V343 Orionis. PASP, 121, 699–707.CrossRefGoogle Scholar
Zacharias, N., Urban, S. E., Zacharius, M. I.et al. (2000). The first US Naval Observatory CCD astrograph catalog. AJ, 120, 2131–2147.CrossRefGoogle Scholar

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

  • References
  • Richard Dodd, Victoria University of Wellington
  • Book: Using SI Units in Astronomy
  • Online publication: 05 December 2011
  • Chapter DOI: https://doi.org/10.1017/CBO9781139019798.014
Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

  • References
  • Richard Dodd, Victoria University of Wellington
  • Book: Using SI Units in Astronomy
  • Online publication: 05 December 2011
  • Chapter DOI: https://doi.org/10.1017/CBO9781139019798.014
Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

  • References
  • Richard Dodd, Victoria University of Wellington
  • Book: Using SI Units in Astronomy
  • Online publication: 05 December 2011
  • Chapter DOI: https://doi.org/10.1017/CBO9781139019798.014
Available formats
×