Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-18T20:38:49.214Z Has data issue: false hasContentIssue false
  • English
  • Français

Supernovae: Progenitor Stars and Mechanisms

Published online by Cambridge University Press:  14 August 2015

J. Craig Wheeler
J. Craig Wheeler*
Affiliation:
Department of Astronomy, University of Texas at Austin

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.

Type II supernovae probably arise predominantly in stars of 8–15 M⊙ which leave neutron star remnants but accomplish little in the way of nucleosynthesis. Stars in the mass range ~ 15-70 M⊙ may either explode or collapse. Their evolution and final outcome, including their contribution to nucleosynthesis, may depend strongly on processes of mass loss. Type I supernovae probably involve a deflagrative explosion in a carbon-oxygen core surrounded by a distended helium envelope. The evolutionary origin of such a configuration is obscure.

Type
Session 7: Supernova Explosions Leading to the Formation of Neutron Stars and Black Holes
Information
Symposium - International Astronomical Union , Volume 93: Fundamental Problems in the Theory of Stellar Evolution , 1981 , pp. 285 - 294
Copyright
Copyright © Reidel 1981 

References

Arnett, W. D.: 1977, Astrophys. J., 218, pp.815.CrossRefGoogle Scholar
Ashworth, W.: 1980, B.A.A.S., 11, pp.660.Google Scholar
Axelrod, T.: 1980, in Supernovae Spectra-Atomic and Spectroscopic Data Needs, ed. Meyerott, R. E. and Gillespie, G. H., in press.Google Scholar
Becker, S. A., and Iben, I. Jr.: 1979, Astrophys. J., 232, pp.831.CrossRefGoogle Scholar
Bethe, H. A., Brown, G. E., Applegate, Jr. and Lattimer, J. M.: 1979, Nuclear Phys. A., 324, pp.487.Google Scholar
Branch, D.: 1980, in Proceedings of the Texas Workshop on Type I Supernovae, ed. Wheeler, J. C. (Univ. of Texas, Austin).Google Scholar
Chevalier, R. A.: 1976, Astrophys. J., 207, pp.872.Google Scholar
Chevalier, R. A.: 1980, preprint.Google Scholar
Chevalier, R. A., and Kirshner, R. P.: 1979, Astrophys. J., 233, pp. 154.CrossRefGoogle Scholar
Chiosi, C., and Caimmi, C.: 1979, Astron. and Astrophys., 74, pp.62.Google Scholar
Colgate, S. A., and Petschek, A. G.: 1980, Astrophys. J. (Letters), 236, pp.L115.Google Scholar
Colgate, S. A., Petschek, A. G., and Kriese, J. T.: 1980, Astrophys. J. Letters, 237, pp.L81.CrossRefGoogle Scholar
Epstein, R. I.: 1979, Monthly Notices Roy. Astron. Soc., 188, pp.305.Google Scholar
Falk, S. W., and Arnett, W. D.: 1977, Astrophys. J. Suppl., 33, pp.515.Google Scholar
Glen, G., and Sutherland, P.: 1980, Astrophys. J., 239, pp.000.CrossRefGoogle Scholar
Helfand, D. J., Chanan, G. A., and Novick, R.: 1980, Nature, 238,p.337.Google Scholar
Kirshner, R. P., Oke, J. B., Penston, M. V., and Searle, S.: 1973a, Astrophys. J., 185, p.303.Google Scholar
Kirshner, R. P., Willner, S. P., Becklin, E.E., Neugebauer, G., and Oke, J. B.: 1973, Astrophys. J. (Letters), 180, p.L97.Google Scholar
Koester, D., and Weidemann, V.: 1980, Astron. and Astrophys., 81,p.145.Google Scholar
Lamb, S. A.: 1978, Astrophys. J., 220, p.186.Google Scholar
Lamb, D. Q., Lattimer, J. M., Pethick, C. J., and Ravenhall, D. G.: 1978, Physics Rev. Letters, 41, p.1623.CrossRefGoogle Scholar
Lichtenstadt, I., Sack, N., and Bludman, S. A.: 1980, Astrophys. J., 237, p.903.Google Scholar
Livio, M., Buchler, J. R., and Colgate, S. A.: 1980, Astrophys. J. (Letters), 238, p.L139.Google Scholar
Maza, J., and van den Bergh, S.: 1976, Astrophys. J., 204, p.519.Google Scholar
Mazurek, T. J.: 1974, Nature, 252, p.287.CrossRefGoogle Scholar
Mazurek, T. J.: 1977, Comments on Astrophys., 7, p.77.Google Scholar
Murray, S. S., Fabbiano, G., Fabian, A. C., Epstein, A., and Giacconi, R.: 1979, Astrophys. J. (Letters), 234, p.L69.Google Scholar
Nomoto, K.: 1980, in Proceedings of the Texas Workshop on Type I Supernovae, ed. Wheeler, J. C. (Univ. of Texas, Austin).Google Scholar
Oemler, A., and Tinsley, B. M.: 1979, Astron. J., 84, p.985.Google Scholar
Romanishin, W., and Angel, J. R. P.: 1980, Astrophys. J., 235, p.992.Google Scholar
Sato, K.: 1975, Prog. Theor. Phys., 53, p.595.Google Scholar
Sneden, C., Lambert, D. L., and Whitaker, R. W.: 1979, Astrophys. J. 234, p.964.Google Scholar
Sparks, W. M., and Endal, E. S.: 1980, Astrophys. J., 237, p.130.CrossRefGoogle Scholar
Sugimoto, D.: 1971, Prog. Theor. Phys., Kyoto, 45, p.761.Google Scholar
Sugimoto, D., and Nomoto, K.: 1980, Space Science Review, 25, p.155.CrossRefGoogle Scholar
Tammann, G. A.: 1978, Mem. Soc. Astron. It., 49, p.315.Google Scholar
Tinsley, B. M.: 1979, Astrophys. J., 229, p.1046.Google Scholar
Tohlin, J. E., Schombert, J. M., and Boss, A. q.: 1980, IAU Colloquium No. 58, Stellar Hydrodynamics Los Alamos.Google Scholar
Tuchman, Y., Sack, N., and Barkat, Z.: 1979, Astrophys. J., 234, p.217.Google Scholar
Vanbeveren, D., and Olson, G. L.: 1980, Astron. and Astrophys., 81,p.228.Google Scholar
Van Riper, K. A., and Arnett, W. D.: 1978, Astrophys. J. (Letters), 225, p.L129.CrossRefGoogle Scholar
Van Riper, K. A., and Lamb, D. Q.: 1980, Astrophys. J. (Letters), 000, p.000.Google Scholar
Weaver, T. A., and Woosley, S. E.: 1980, B.A.A.S., 11, p.724.Google Scholar
Weaver, T. A., and Woosley, S. E.: 1980, Ann. N.Y. Acad. Sci., 336, p.335.Google Scholar
Weaver, T. A., Zimmerman, G. B., and Woosley, S. E.: 1978, Astrophys. J. 225, p.1021.Google Scholar
Wheeler, J. C.: 1980, Proceedings of the Texas Workshop on Type I Supernovae, ed. Wheeler, J. C., (Univ. of Texas, Austin).Google Scholar
Wheeler, J. C.: 1981, Reports on Progress in Physics, in press.Google Scholar
Woosley, S. E., Weaver, T. A., and Taam, R. E.: 1980, Proceedings of The Texas Workshop on Type I Supernovae, ed. Wheeler, J. C. (Univ. of Texas, Austin).Google Scholar