Hostname: page-component-cd9895bd7-dzt6s Total loading time: 0 Render date: 2024-12-23T11:51:06.916Z Has data issue: false hasContentIssue false
  • English
  • Français

Developments in Physics of Massive Stars

Published online by Cambridge University Press:  01 December 2007

Georges Meynet ,
Sylvia Ekström ,
André Maeder ,
Raphael Hirschi ,
Cyril Georgy  and
Coralie Beffa
Georges Meynet
Affiliation:
Observatory of Geneva University, Switzerland email (G. Meynet): [email protected]
Sylvia Ekström
Affiliation:
Observatory of Geneva University, Switzerland email (G. Meynet): [email protected]
André Maeder
Affiliation:
Observatory of Geneva University, Switzerland email (G. Meynet): [email protected]
Raphael Hirschi
Affiliation:
EPSAM, University of Keele, UK email: [email protected]
Cyril Georgy
Affiliation:
Observatory of Geneva University, Switzerland email (G. Meynet): [email protected]
Coralie Beffa
Affiliation:
Observatory of Geneva University, Switzerland email (G. Meynet): [email protected]
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.

New constraints on stellar models are provided by large surveys of massive stars, interferometric observations and asteroseismology. After a review of the main results so far obtained, we present new results from rotating models and discuss comparisons with observed features. We conclude that rotation is a key feature of massive star physics.

Keywords

stars: abundances – stars: early-type – stars: evolution – stars: mass loss – stars: emission-lineBe – stars: rotation – gamma rays: bursts
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S250: Massive Stars as Cosmic Engines , December 2007 , pp. 147 - 160
Copyright
Copyright © International Astronomical Union 2008

References

Asplund, M., Grevesse, N., & Sauval, A. J. 2005, in: Barnes, T. G. III & Bash, F. N. (eds.), Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis, (San Francisco: ASP), ASP Conf. Ser., 336 25Google Scholar
Domiciano de Souza, A., Driebe, T., & Chesneau, O. 2007, AJ, 464, 81Google Scholar
Dufton, P. L., Smartt, S. J., Lee, J. K., et al. 2006, A&A, 457, 265Google Scholar
Ekström, S., Meynet, G., Maeder, A. & Barblan, F. 2008, A&A, 478, 467Google Scholar
Eldridge, J. J. & Vink, J. S. 2006, A&A, 452, 295Google Scholar
Eldridge, J. J., Izzard, R. G., & Tout, C. A. 2008, MNRAS, 384, 1109CrossRefGoogle Scholar
Evans, C. J., Smartt, S. J., Lee, J.-K., et al. 2005, A&A, 437, 467Google Scholar
Evans, C. J., Lennon, D. J., Smartt, S. J., & Trundle, C. 2006, A&A, 456, 623Google Scholar
Heap, S. R., Lanz, T., & Hubeny, I. 2006, ApJ, 638, 409CrossRefGoogle Scholar
Herrero, A., Kudritzki, R. P., Vilchez, J. M., et al. 1992, A&A, 261, 209Google Scholar
Huang, W. & Gies, D. R. 2006a, ApJ, 648, 580CrossRefGoogle Scholar
Huang, W. & Gies, D. R. 2006b, ApJ, 648, 591CrossRefGoogle Scholar
Hunter, I., Dufton, P. L., Smartt, S. J., et al. 2007, A&A, 466, 277Google Scholar
Hunter, I., Lennon, D. J., Dufton, P. L., et al. 2008a A&A, 479, 541Google Scholar
Hunter, I., Brott, I., Lennon, D. J., et al. 2008b ApJ, 676, L29CrossRefGoogle Scholar
Keller, S. 2004, PASA, 21, 310CrossRefGoogle Scholar
Kervella, P. & Domiciano de Souza, A. 2006, A&A, 453, 1059Google Scholar
Kervella, P. & Domiciano de Souza, A. 2007, A&A, 474, 49Google Scholar
Lyubimkov, L. S., Rostopchin, S. I., & Lambert, D. L. 2004, MNRAS, 351, 745CrossRefGoogle Scholar
Maeder, A. 1999, A&A, 347, 185Google Scholar
Maeder, A. & Meynet, G. 2001, A&A, 373, 555Google Scholar
Maeder, A., Grebel, E. K., & Mermilliod, J.-C. 1999, A&A, 346, 459Google Scholar
Martayan, C., Frémat, Y., Hubert, A.-M., et al. 2006, A&A, 452, 273Google Scholar
Martayan, C., Floquet, M., Hubert, A.-M., et al. 2007a A&A, 472, 577Google Scholar
Martayan, C., Frémat, Y., Hubert, A.-M., et al. 2007b A&A, 462, 683Google Scholar
Meilland, A., Millour, F., & Stee, P. 2007a A&A, 464, 73Google Scholar
Meilland, A., Stee, P., & Vannier, M. 2007b A&A, 464, 59Google Scholar
Meynet, G. & Maeder, A. 2005, A&A, 429, 581Google Scholar
Meynet, G. & Maeder, A. 2007, A&A, 464, L11Google Scholar
Meynet, G., Ekström, S., & Maeder, A. et al. 2008, in: Abel, T., Heger, A. & O'Shea, B. (eds.), First Stars III, (New York: AIP), in press (arXiv:0709.2275)Google Scholar
Millour, F., Petrov, R. G., & Chesneau, O. 2007, A&A, 464, 107Google Scholar
Mokiem, M. R., de Koter, A., Evans, C. J., et al. 2006, A&A, 456, 1131Google Scholar
Mokiem, M. R., de Koter, A., Evans, C. J., et al. 2007, A&A, 465, 1003Google Scholar
Strom, S. E., Wolff, S. C., & Dror, D. H. A. 2005, AJ, 129, 809CrossRefGoogle Scholar
Trundle, C., Dufton, P. L., Hunter, I., et al. 2007, A&A, 471, 625Google Scholar
Vink, J. S., de Koter, A., & Lamers, H. J. G. L. M. 2001, A&A, 369, 574Google Scholar
Weigelt, G., Kraus, S., & Driebe, T. 2007, A&A, 464, 87Google Scholar
Wisniewski, J. P., & Bjorkman, K. S. 2006, ApJ, 652, 458CrossRefGoogle Scholar
Wolff, S. C., Strom, S. E., Dror, D., & Venn, K. 2007, AJ, 133, 1092CrossRefGoogle Scholar