Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-24T13:56:44.396Z Has data issue: false hasContentIssue false
  • English
  • Français

The most massive AGB stars

Published online by Cambridge University Press:  01 April 2008

Lionel Siess
Lionel Siess*
Affiliation:
Institut d'Astronomie et d'Astrophysique, Université libre de Bruxelles, 1050 Bruxelles, Belgium email: [email protected] Centre for Stellar and Planetary Astrophysics, School of Mathematical Sciences, Monash University, Victoria 3800, Australia
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.

The general properties of stars in the mass range 7–12M⊙, also referred to as super-AGB stars, are reviewed and special attention is paid to determine how their mass range depends on the initial metallicity and what fraction of these stars end their life as ONe white dwarfs or explode as electron-capture supernova.

Keywords

Stars: AGB and post-AGBstars: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S252: The Art of Modeling Stars in the 21st Century , April 2008 , pp. 297 - 307
Copyright
Copyright © International Astronomical Union 2008

References

Baron, E., Cooperstein, J., & Kahana, S. 1987, ApJ, 320, 300Google Scholar
Bethem, H. A. & Wilson, J. R. 1985, ApJ, 295, 14CrossRefGoogle Scholar
Canal, R., Isern, J, & Labay, J. 1992, ApJ, 398, 49CrossRefGoogle Scholar
Chiappini, C., Ekstrm, S., Meynet, G. et al. 2008, A&A, 479, L9Google Scholar
Chiappini, C., Matteucci, F., & Ballero, S. K. 2005, A&A, 437, 429Google Scholar
de Jager, C., Nieuwenhuijzen, H., & van der Hucht, K. A. 1988, A&AS, 72, 259Google Scholar
Dessart, L., Burrows, A., Ott, C. D., et al. 2003, ApJ, 644, 1063Google Scholar
Doherty, C. L. & Lattanzio, J. C. 2006, MmSAI 77, 828Google Scholar
Eldridge, J. J. & Tout, C. A. 2004, MNRAS, 353, 87Google Scholar
Gil-Pons, P., García-Berro, E., José, J., Hernanz, M., & Truran, J. W. 2003, A&A, 407, 1021Google Scholar
Gil-Pons, P., Suda, T., Fujimoto, M. Y. & García-Berro, E. 2005, A&A, 433, 1037Google Scholar
Gil-Pons, P., Gutiérrez, J., & García-Berro, E. 2007, A&A, 464, 667Google Scholar
García-Berro, E. & Iben, I. 1994, ApJ, 434, 306CrossRefGoogle Scholar
García-Berro, E., Ritossa, C., & Iben, I. 1997, ApJ, 485, 765Google Scholar
Gutiérrez, J., Canal, R., & García-Berro, E. 2005, A&A, 435, 231Google Scholar
Gutiérrez, J., García-Berro, E., Iben, I., et al. 1996, ApJ, 459, 701Google Scholar
Habets, G. M. H. J. 1986, A&A, 167, 61 ApJ, 489, 772Google Scholar
Hendry, M. A., Smartt, S. J., Maund, J. R., et al. 2005, MNRAS, 359, 906CrossRefGoogle Scholar
Hendry, M. A., Smartt, S. J., Crockett, R. M., et al. 2006, MNRAS, 369, 1303CrossRefGoogle Scholar
Hoffman, R. D., Mller, B., & Janka, H.-T 2008, ApJ, 676, L127Google Scholar
Iben, I., Ritossa, C., & García-Berro, E. 1997Google Scholar
Imbriani, G., Limongi, M., Gialanella, L., Straniero, O., & Chieffi, A. 2001, ApJ, 558, 903CrossRefGoogle Scholar
Janka, H.-T, Mller, B., Kitaura, F. S., & Buras, R. 2008, A&A, in pressGoogle Scholar
José, J. & Hernanz, M. 1998, ApJ, 494, 680Google Scholar
Kitaura, F. S., Janka, H.-Th., & Hillebrandt, W. 2006, A&A, 450, 345Google Scholar
Kudritzki, R. P., Pauldrach, A., & Puls, J. 1987, A&A, 173, 293Google Scholar
Li, W., Wang, X., Van Dyk, S. D., et al. 2007, ApJ, 661, 1013CrossRefGoogle Scholar
Liebert, J., Bergeron, P., & Holberg, J. B. 2005, ApJS, 156, L47CrossRefGoogle Scholar
Maund, J. R., Smartt, S. J., & Danziger, I. J. 2005, MNRAS, 364, L33Google Scholar
Mayle, R. & Wilson, J. R. 1988, ApJ, 334, 909Google Scholar
Miyaji, S., Nomoto, K., Yokoi, K., & Sugimoto, D. 1980, Publ. Astron. Soc. Japan, 32, 303Google Scholar
Ning, H., Qian, Y.-Z., & Meyer, B. S. 2007, ApJ, 667, L159CrossRefGoogle Scholar
Nomoto, K. 1981, IAU Symp., 93, 295Google Scholar
Nomoto, K. 1984, ApJ, 277, 791Google Scholar
Nomoto, K. 1987, ApJ, 322, 206Google Scholar
Pfahl, E., Rappaport, S., Podsiadlowski, P., et al. 2002, ApJ, 574, 364CrossRefGoogle Scholar
Podsiadlowski, Ph., Langer, N., Poelarends, A. J. T., et al. 2004, ApJ, 612, 1044Google Scholar
Poelarends, A. J. T., Herwig, F., Langer, N., & Heger, A. 2008, ApJ, 675, 614CrossRefGoogle Scholar
Ritossa, C., García-Berro, E., & Iben, I. 1996, ApJ, 460, 489CrossRefGoogle Scholar
Ritossa, C., García-Berro, E., & Iben, I. 1999, ApJ, 515, 381CrossRefGoogle Scholar
Sackmann, I.-J. & Boothroyd, A. I. 1991, ApJ, 366, 529Google Scholar
Siess, L. 2006, A&A, 448, 717Google Scholar
Siess, L. 2007, A&A, 476, 893Google Scholar
Siess, L. & Arnould, M. 2008, A&A, submittedGoogle Scholar
Timmes, F. X. & Woosley, S. E. 1992, ApJ, 396, 649Google Scholar
Vassiliadis, E. & Wood, P. R. 1993, ApJ, 413, 641Google Scholar
Ventura, P. & D'Antona, F. 2005, A&A, 431, 279Google Scholar