Hostname: page-component-76fb5796d-22dnz Total loading time: 0 Render date: 2024-04-26T12:41:11.650Z Has data issue: false hasContentIssue false
  • English
  • Français

Two Centuries of Study of Algol Systems

Published online by Cambridge University Press:  12 April 2016

Alan H. Batten
Alan H. Batten*
Affiliation:
Dominion Astrophysical Observatory,Herzberg Institute of Astrophysics,5071 W. Saanich Road, Victoria B.C. V8X 4M6,Canada

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.

The periodicity of the light variation of Algol, discovered just over 200 years ago, may be regarded as the beginning of the study of eclipsing binary systems, especially those of the Algol type. Such studies, however, gained no real momentum until Vogel, 100 years ago, demonstrated by spectroscopy that the binary hypothesis of Algol’s light changes is, in its essentials, correct. Three elements were needed to give us our modern notions of evolution by mass-transfer, namely: (i) results of combined analysis of light-curves and velocity-curves, (ii) evidence of circumstellar matter within binary systems and (iii) the notion that at least one component of an Algol system was near the limit of dynamical stability. All three entered the literature within about a decade, approximately halfway through the second century of eclipsing-binary studies; but it is the computational and instrumental developments of the last 25 years that have made real progress possible. We still lack commensurate theoretical developments, and the whole question of the contribution of Algol systems to the development of the Galaxy has barely been considered.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 107: Algols , 1989 , pp. 1 - 8
Copyright
Copyright © Kluwer 1989

References

Aitken, R.G. 1935, The Binary Stars McGraw-Hill Book Co., New York, p. 3 (Dover Reprint 1964).Google Scholar
Audouze, J. and Tinsley, B.M. 1976, Ann. Rev. Astron. Astrophys. 14, 23.Google Scholar
Batten, A.H. 1981, in Investigating the Universe ed. Kahn, F.D., D. Reidel, Dordrecht, Holland, p. 207.Google Scholar
Batten, A.H. 1988, Publ. Astr. Soc. Pacific 100, 160.Google Scholar
Biermann, P. 1971, Astron. Astrophys. 10, 205.Google Scholar
Budding, E. 1984, Bull. d’Inf. Centre Données Stellaires 27, 91.Google Scholar
Budding, E. 1988, Southern Stars 32, 180.Google Scholar
Carpenter, E.F. 1930, Astrophys. J. 72, 205.Google Scholar
Crawford, J.A. 1955, Astrophys. J. 121, 71.Google Scholar
Dugan, R.S. 1920, Contr. Princeton Obs. No. 5.Google Scholar
Eggen, O.J. 1957, Observatory 77, 191.Google Scholar
Garrison, R.F., Schild, R.E., Hiltner, W.A. and Krzemiski, W. 1984, Astrophys. J. 276, L13.Google Scholar
Giuricin, G., Mardirossian, F. and Mezzetti, M. 1983, Astrophys. J. Suppl. 52, 35.Google Scholar
Goodricke, J. 1783, Phil. Trans. Roy. Soc. 73, 474.Google Scholar
Hoskin, M.A. 1979, J. Hist. Astron. 10, 23.Google Scholar
Hoyle, F. 1955, Frontiers of Astronomy, Wm Heinemann, London, pp. 195–202.Google Scholar
Jeffreys, H. 1964, Quarterly J. Roy. Astron. Soc. 5, 10.Google Scholar
Joy, A.H. 1942, Publ. Astr. Soc. Pacific 54, 35.Google Scholar
Kondo, Y., McCluskey, G.E. and Stencel, R.E. 1980, Astrophys. J. 233, 906.Google Scholar
Kopal, Z. 1957, in Non-Stable Stars ed. Herbig, G.H., Cambridge Univ. Press, p. 123.Google Scholar
Kopal, Z. 1959, Close Binary Systems, Chapman and Hall London, pp. 1–5.Google Scholar
Kopal, Z. 1971, Publ. Astron. Soc. Pacific 83, 521.Google Scholar
Kopal, Z. 1978, Dynamics of Close Binary Systems, D. Reidel, Dordrecht, Holland, Chap. 8.Google Scholar
Kruszewski, A. 1964, Acta Astr. 14, 214.Google Scholar
Kuiper, G.P. 1941, Astrophys. J. 93, 133.CrossRefGoogle Scholar
Lubow, S.H. and Shu, F.H. 1975, Astrophys. J. 198, 383.Google Scholar
Mayer, C. 1779, De novis in Coelo Sidereo Phaenominis in miris Stellarum fixarum Comitibus.Google Scholar
Micheli, J. 1767, Phil. Trans. Roy. Soc. 57, 234.Google Scholar
Paczynski, B. 1971, Ann. Rev. Astron. Astrophys. 9, 183.Google Scholar
Parthasarathy, M., Lambert, D.L. and Tomkin, J. 1983, Mon. Not. Roy. Astron. Soc. 203, 1063.Google Scholar
Plavec, M. 1970, Publ. Astron. Soc. Pacific 82, 957.Google Scholar
Plavec, M. 1973, in Extended Atmospheres and Circumstellar Matter in Close Binary Systems, I.A.U. Symp. 52 ed. Batten, A.H., D. Reidel, Dordrecht, Holland, p. 216.Google Scholar
Plavec, M.J. 1983, Astrophys. J. 275, 251.Google Scholar
Prendergast, K.H. and Taam, R.E. 1974, Astrophys. J. 189, 125.Google Scholar
Struve, O. 1949, Mon. Not. Roy. Astron. Soc. 109, 487.Google Scholar
Tinsley, B.M. 1980, Fundamentals of Cosmic Phys. 5, 287.Google Scholar
Vogel, H.C. 1789, Sitzungsber. Prüss. Akad. p. 1045.Google Scholar
Walter, K. 1931, Veröff. Königsberg Sternw. No. 2.Google Scholar
Wood, F.B. 1950, Astrophys. J. 112, 196.Google Scholar