Hostname: page-component-7bb8b95d7b-cx56b Total loading time: 0 Render date: 2024-10-06T13:10:06.605Z Has data issue: false hasContentIssue false
  • English
  • Français

Secular Mass Loss from Cataclysmic Variables

Published online by Cambridge University Press:  12 April 2016

Józef Smak
Józef Smak*
Affiliation:
N. Copernicus Astronomical Center, Polish Academy of Sciences, Aleje Ujazdowskie 4, 00-478 Warszawa, POLAND

Extract

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 mass loss from cataclysmic binaries seems an important and worth studying phenomenon for a number of reasons. It is probably enough to mention only two of them:

(a) Whenever we can directly observe the ejected material, determine its amount and the rate of mass loss, as well as its chemical composition (this being the case of the expanding envelopes of novae), we are getting a good insight into the basic physical mechanisms responsible for the observed phenomena.

(b) The mass loss (together with the mass transfer) and the loss of the orbital angular momentum are related directly to the dynamical evolution of a binary system and - indirectly - to the evolution of its components.

Type
Part II: Cataclysmic Variables
Information
International Astronomical Union Colloquium , Volume 42: The Interaction of Variable Stars with their Environment , 1977 , pp. 365 - 370
Copyright
Copyright © Veröff. Der Remeis-Sterwarte 1977

References

Arnold, S., Berg, R.A., and Duthie, J.G. 1976, Ap.J., 206, 790 Google Scholar
Bielicki, M., Piotrowski, S., and Ziolkowski, K. 1974, Astrophys. Space Sci., 206, 173 Google Scholar
Lin, D.N.C. 1977, Mon.Not.R.Astr.Soc., 179, 265 Google Scholar
Lin, D.N.C., and Pringle, J.E. 1976, IAÜ Symp. No. 73: Structure and Evolution of Close Binary Systems, ed. Eggleton, P., Hitton, S., and Whelan, J. (Dordrecht: D. Reidel), p. 237 Google Scholar
Osaki, Y. 1974, Pub.Astr. Soc. Japan, 26, 429 Google Scholar
Papaloizou, J. and Pringle, J.E. 1977, preprintGoogle Scholar
Pottasch, S.R. 1967, Bull. Astr. Soc. Neth., 19, 227 Google Scholar
Pringle, J.E. 1975, Mon.Not.R.Astr.Soc., 170, 633 CrossRefGoogle Scholar
Robinson, E.L. 1973, Ap.J., 186, 347 Google Scholar
Robinson, E.L. 1976, Ann.Rev.Astr.Astrophys., 14, 119 Google Scholar
Robinson, E.L., Nather, E.R., and Patterson, J. 1977, preprintGoogle Scholar
Smak, J., 1971, IAU Coll. No 15: New Directions and Hew Frontiers in Variable Stars Research (Bamberg: Remeis sternwarte), p. 248 Google Scholar
Smak, J. 1976, Acta Astr., 26, 277 Google Scholar
Warner, B. 1974, Mon.Not.Astr.Soc.S.Africa, 33, 133 Google Scholar