Hostname: page-component-5c6d5d7d68-wpx84 Total loading time: 0 Render date: 2024-08-22T15:16:41.633Z Has data issue: false hasContentIssue false
  • English
  • Français

Evolution of massive close binaries, compared to observations

Published online by Cambridge University Press:  25 May 2016

Dany Vanbeveren
Dany Vanbeveren*
Affiliation:
Astrophysical Institute, Vrije Universiteit Brussel, Pleinlaan 2, B-1050 Brussels, Belgium

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.

Since binaries can not be considered separately from single stars, we first present a brief summary of massive single star evolution. Next, we highlight massive close binary evolutionary facts that are important when massive close binaries are included in population (number) synthesis. Finally, we consider a few interesting test cases.

Type
Part 2. Models for single star evolution of massive stars: wind + atmosphere + interior
Information
Symposium - International Astronomical Union , Volume 193: Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies , 1999 , pp. 196 - 204
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Bhattacharya, D., Wijers, R., Hartman, J., Verbunt, F. 1992, A&A 254, 198 Google Scholar
Biehle, G. 1991, ApJ 380, 167 Google Scholar
Blaauw, A. 1961, Bull. Astron. Inst. Netherlands 15, 265 Google Scholar
Bonnet-Bidaud, J., Chardin, G. 1988, Physics Reports 170, 325 CrossRefGoogle Scholar
Braun, H., Langer, N. 1995a, A&A 297, 483 Google Scholar
Braun, H., Langer, N. 1995b, in: van der Hucht, K.A. & Williams, P.M. (eds.), Wolf-Rayet Stars: Binaries, Colliding Winds, Evolution, Proc. IAU Symp. No. 163 (Dordrecht: Kluwer), p. 305 Google Scholar
Cannon, R., Eggleton, P., Zytkov, A., Podsiadlowski, Ph. 1992, ApJ 386, 206 CrossRefGoogle Scholar
Davidson, K., Ostriker, J. 1973, ApJ 179, 585.Google Scholar
Drissen, L., Lamontagne, R., Moffat, A.F.J., et al. 1986, ApJ 343, 426 Google Scholar
Halbwachs, J. 1987, A&A 183, 234 Google Scholar
Hogeveen, S. 1992, ApSS. 196, 299 Google Scholar
Iben, I., Tutukov, A., Yungelson, Y. 1995, ApJS 100, 217 CrossRefGoogle Scholar
Illarionov, A., Sunyaev, R. 1975, A&A 39, 185 Google Scholar
Jura, M. 1987, ApJ 313, 743 Google Scholar
Leonard, P., Duncan, M. 1988, AJ 96, 222 CrossRefGoogle Scholar
Leonard, P., Duncan, M. 1990, AJ 99, 608 Google Scholar
Lorimer, D., Bailes, M., Harrison, P. 1997, MNRAS 289, 592 Google Scholar
Meynet, G., Maeder, A., Schaller, G., et al. 1994, A&AS 103, 97 Google Scholar
Neo, S., Miyaji, S., Nomoto, K., Sugimoto, D. 1977, PASJ 29, 249 Google Scholar
Petrenz, P., Puls, J. 1996, A&A 312, 195 Google Scholar
Podsiadlowski, Ph., Joss, P., Hsu, J. 1992, ApJ. 391, 246 Google Scholar
Popova, E., Tutukov, A., Yungelson, L. 1982, ApSS 88, 55 Google Scholar
Puls, J., Kudritzki, R., Herrero, A., et al. 1996, A&A 305, 171 Google Scholar
Schaller, G., Schaerer, D., Meyent, G., Maeder, A. 1992, A&AS 96, 269 Google Scholar
Schmutz, W., Geballe, T., Schild, H. 1996, A&A 311, L25 Google Scholar
Stevens, I., Willis, A. 1988, MNRAS 234, 783 Google Scholar
Thorne, K., Zytkov, A. 1977, ApJ 212, 862 Google Scholar
Vanbeveren, D., van Rensbergen, W., de Loore, C. 1982, A&A 115, 68 Google Scholar
Vanbeveren, D., de Loore, C. 1994, A&A 290, 129 Google Scholar
Vanbeveren, D., Herrero, A., Kunze, D., Van Kerkwijk, M. 1994, SSR 66, 395 Google Scholar
Vanbeveren, D., van Rensbergen, W., de Loore, C. 1998a, The Brightest Binaries (Dordrecht: Kluwer)Google Scholar
Vanbeveren, D., De Donder, E., Van Bever, J., et al. 1998b, New Astronomy 3, 443 Google Scholar
Vanbeveren, D., de Loore, C., van Rensbergen, W. 1998c, The A&A Review 9, 63 Google Scholar
Vereshchagin, S., Kraicheva, Z., Popova, E., et al. 1987, PAZh 13, 63 Google Scholar
Vereshchagin, S., Tutukov, A., Yungelson, L., et al. 1988, ApSS 142, 245 Google Scholar
Webbink, R. 1984, ApJ 277, 355 CrossRefGoogle Scholar
Woosley, S.E.: 1986, in: Hauck, B. et al. (eds.), Nucleosynthesis and Chemical Evolution, Proc. 16th Saas-Fee Course (Geneva: Geneva Observatory), p. 1 Google Scholar