Hostname: page-component-745bb68f8f-b95js Total loading time: 0 Render date: 2025-01-11T07:06:08.209Z Has data issue: false hasContentIssue false
  • English
  • Français

Rotation and Massive Close Binary Evolution

Published online by Cambridge University Press:  01 December 2007

Norbert Langer ,
Matteo Cantiello ,
Sung-Chul Yoon ,
Ian Hunter ,
Ines Brott ,
Danny Lennon ,
Selma de Mink  and
Marcel Verheijdt
Norbert Langer
Affiliation:
Astronomical Institute, Utrecht University, The Netherlands
Matteo Cantiello
Affiliation:
Astronomical Institute, Utrecht University, The Netherlands
Sung-Chul Yoon
Affiliation:
University of California, Santa Cruz, USA
Ian Hunter
Affiliation:
The Queen's University of Belfast, Northern Ireland, UK
Ines Brott
Affiliation:
Astronomical Institute, Utrecht University, The Netherlands
Danny Lennon
Affiliation:
Isaac Newton Group, Santa Cruz de La Palma, Canary Islands, Spain
Selma de Mink
Affiliation:
Astronomical Institute, Utrecht University, The Netherlands
Marcel Verheijdt
Affiliation:
Astronomical Institute, Utrecht University, The Netherlands
Rights & Permissions [Opens in a new window]

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.

We review the role of rotation in massive close binary systems. Rotation has been advocated as an essential ingredient in massive single star models. However, rotation clearly is most important in massive binaries where one star accretes matter from a close companion, as the resulting spin-up drives the accretor towards critical rotation. Here, we explore our understanding of this process, and its observable consequences. When accounting for these consequences, the question remains whether rotational effects in massive single stars are still needed to explain the observations.

Keywords

stars: early-type – stars: fundamental parameters – stars: mass loss – stars: rotation – stars: binaries: close
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S250: Massive Stars as Cosmic Engines , December 2007 , pp. 167 - 178
Copyright
Copyright © International Astronomical Union 2008

References

Berger, L., Koester, D., Napiwotzki, R., et al. 2005, A&A, 444, 565Google Scholar
Belczynski, K., Kalogera, V., & Bulik, T. 2002, ApJ, 572, 407CrossRefGoogle Scholar
Bradley, P. A. 1998, ApJS, 116, 307CrossRefGoogle Scholar
Bradley, P. A. 2001, ApJ, 552, 326CrossRefGoogle Scholar
Braun, H. & Langer, N. 1995, A&A, 297, 483Google Scholar
Brinkworth, C. S., Burleigh, M. R., & Marsh, T. R. 2007, in: Napiwotzki, R. & Burleigh, M. R. (eds.), 15th European Workshop on White Dwarfs (San Francisco: ASP), ASP Conf. Ser., 372, 183Google Scholar
Camilo, F., Ransom, S. M., Halpern, J. P., & Reynolds, J. 2007, ApJ, 666, L93CrossRefGoogle Scholar
Cantiello, M., Yoon, S.-C., Langer, N., & Livio, M. 2007, A&A, 465, L29Google Scholar
Detmers, R., Langer, N., Podsiadlowski, P., & Izzard, R. 2008, A&A, in press, astro-ph/0804.0014Google Scholar
Dolez, N., Vauclair, G., Kleinman, S. J., et al. 2006, A&A, 446, 237Google Scholar
Eldridge, J. J., Izzard, R. G., Tout, C. A. 2008, 384, 1109CrossRefGoogle Scholar
Evans, C. J., Smartt, S. J., Lee, J.-K., et al. 2005, A&A, 437, 467Google Scholar
Ferrario, L. & Wickramasinghe, D. T. 2005, MNRAS, 356, 615CrossRefGoogle Scholar
Handler, G. 2001, MNRAS, 323, L43CrossRefGoogle Scholar
Handler, G., Romero-Colmenero, E., & Montgomery, M. H. 2002, MNRAS, 335, 399CrossRefGoogle Scholar
Heger, A. & Langer, N. 2000, ApJ, 544, 1016CrossRefGoogle Scholar
Heger, A., Langer, N., & Woosley, S. E. 2000, ApJ, 528, 368CrossRefGoogle Scholar
Heger, A., Woosley, S. E., & Spruit, H. C. 2005, ApJ, 626, 350CrossRefGoogle Scholar
Hunter, I., Brott, I., Lennon, D. J., et al. , 2008, ApJ, 676, L29CrossRefGoogle Scholar
Kepler, S. O., Giovannini, O., Wood, M. A., et al. 1995, ApJ, 447, 874CrossRefGoogle Scholar
Kleinman, S. J., Nather, R. E., Winget, D. E., et al. 1998, ApJ, 495, 424CrossRefGoogle Scholar
Langer, N. 1998, A&A, 329, 551Google Scholar
Maeder, A. & Meynet, G. 2000, ARAA, 38, 143CrossRefGoogle Scholar
Maeder, A. & Meynet, G. 2005, A&A, 440, 1041Google Scholar
Meynet, G. & Maeder, A. 2000, A&A, 361, 101Google Scholar
Mokiem, M. R., de Koter, A., Evans, C. J., et al. 2006, A&A, 456, 1131Google Scholar
Packet, W. 1981, A&A, 102, 17Google Scholar
Petrovic, J., Langer, N., Yoon, S.-C., & Heger, A. 2005a A&A, 435, 247Google Scholar
Petrovic, J., Langer, N., & van der Hucht, K. A. 2005b A&A, 435, 1013Google Scholar
Podsiadlowski, P., Joss, P. C., & Hsu, J. J.L. 1992, ApJ, 391, 246CrossRefGoogle Scholar
Pols, O. R. & Marinus, M. 1994, A&A, 288, 475Google Scholar
Spruit, H. C. 2002, A&A, 381, 923Google Scholar
Suijs, M. P. L., Langer, N., Poelarends, A.-J., et al. 2008, A&A, 481, L87Google Scholar
Vanbeveren, D., Van Bever, J., & Belkus, H. 2007, ApJ, 662, L107CrossRefGoogle Scholar
Vazquez, G. A., Leitherer, C., Schaerer, D., et al. 2007, ApJ, 663, 995CrossRefGoogle Scholar
Wellstein, S. 2001, PhD thesis, University PotsdamGoogle Scholar
Wellstein, S. & Langer, N. 1999, A&A, 350, 148Google Scholar
Wellstein, S., Langer, N., & Braun, H. 2001, A&A, 369, 939Google Scholar
Winget, D. E., Nather, R. E., & Clemens, J. C. 1994, ApJ, 430, 839CrossRefGoogle Scholar
Woosley, S. E. & Heger, A. 2006, ApJ, 637, 914CrossRefGoogle Scholar
Yoon, S.-C. & Langer, N. 2005, A&A, 443, 643Google Scholar
Yoon, S.-C., Langer, N., & Norman, C. 2006, A&A, 460, 199Google Scholar