Hostname: page-component-78c5997874-j824f Total loading time: 0 Render date: 2024-11-04T19:30:46.197Z Has data issue: false hasContentIssue false

Supernova Abundance Generation

Published online by Cambridge University Press:  19 July 2016

K. Nomoto
Affiliation:
Department of Astronomy, Faculty of Science, University of Tokyo, Tokyo 113
T. Shigeyama
Affiliation:
Department of Astronomy, Faculty of Science, University of Tokyo, Tokyo 113
T. Tsujimoto
Affiliation:
Department of Astronomy, Faculty of Science, University of Tokyo, Tokyo 113

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.

Theoretical models of supernova explosions of various types are reviewed to obtain heavy element yields from supernovae. We focus on new models for SN 1987A, and Type Ia, Ib, and Ic supernovae. Maximum brightness and decline rate of their light curves suggest that 12–18 M stars produce larger amount of 56Ni than more massive stars. We discuss relative roles of various types of supernovae in the chemical evolution of galaxies.

Type
Setting the Stage
Copyright
Copyright © Kluwer 1991 

References

Anders, E., and Grevesse, N. 1989, Geochim. Cosmochim. Acta , 53, 197.Google Scholar
Andersen, J., Edvardsson, B., Gustafsson, B., and Nissen, P.E. 1988, in IAU Symp. 132, The Impact of Very High S/N Spectroscopy on Stellar Physics , ed. Cayrel, G., de Strobel, M. Spite (Dordrecht: Kluwer), p.441.Google Scholar
Arnett, W.D. 1988, Ap. J., 334, 500.Google Scholar
Arnett, W.D., Bahcall, J.N., Kirshner, R.P., and Woosley, S.E. 1989, Ann. Rev. Astr. Ap. , 27, 629.Google Scholar
Axelrod, T. 1980, in Type I Supernovae , ed. Wheeler, J.C. (Univ. of Texas), p. 80.Google Scholar
Barbuy, B. 1988, Astr. Ap. , 191, 121.Google Scholar
Begelman, M.C., and Sarazin, C.L. 1986, Ap. J. (Letters) , 302, L59.Google Scholar
Bouchet, P., Danziger, I.J., and Lucy, L. 1990, in SN 1987A and Other Supernovae , ed. Danziger, I.J. (Garching: ESO), in press.Google Scholar
Branch, D. 1986, Ap. J. (Letters) , 300, L51.Google Scholar
Branch, D., Doggett, J.B., Nomoto, K., and Thielemann, F.-K. 1985, Ap. J. , 294, 619.CrossRefGoogle Scholar
Catchpole, R. et al. 1987, M. N. R. A. S. , 229, 15p.Google Scholar
Danziger, I.J., Lucy, L.B., and Bouchet, , 1990, in Supernovae , ed. Woosley, S.E. (Springer-Verlag), in press.Google Scholar
Elias, J.H. et al. 1990, in SN 1987A and Other Supernovae , ed. Danziger, I.J. (Garching: ESO), in press.Google Scholar
Evans, R., van den Bergh, S., McClure, R.D. 1989, Ap. J. 345, 752 Google Scholar
Ensman, L., and Woosley, S.E. 1988, Ap. J. , 333, 754.Google Scholar
Filippenko, A.V. 1988, A. J. , 96, 1941.Google Scholar
Filippenko, A.V., Porter, A.C., and Sargent, W.L.W. 1990, A. J. , 100, 1575.Google Scholar
Gaskell, C.M., Cappellaro, E., Dinerstein, H.L., Garnett, D.R., Harkness, R.P., and Wheeler, J.C. 1986, Ap. J. (Letters) , 306, L77.Google Scholar
Graham, J.R. 1987, Ap. J. , 315, 588.Google Scholar
Gratton, R.G. 1990, this volume.Google Scholar
Gratton, R.G., and Ortolani, S. 1986, Astr. Ap. , 169, 201.Google Scholar
Hachisu, I., Kato, M., and Saio, H. 1989, Ap. J. (Letters) , 342, L19.Google Scholar
Hachisu, I., Matsuda, T., Nomoto, K., and Shigeyama, T. 1991, Ap. J. (Letters) , in press.Google Scholar
Harkness, R.P., and Wheeler, J.C. 1990, in Supernovae , ed. Petschek, A. (Springer-Verlag), p. 1.Google Scholar
Hashimoto, M., Nomoto, K., and Shigeyama, T. 1988, Astr. Ap. , 210, L5.Google Scholar
Iben, I. Jr., and Tutukov, A. 1984, Ap. J. Suppl. , 55, 335.Google Scholar
Jeffery, D., Brauch, D., Filippenko, A.V., and Nomoto, K. 1990, preprint.Google Scholar
Kumagai, S., Shigeyama, T., Nomoto, K., Itoh, M., Nishimura, J., and Tsuruta, S. 1989, Ap. J. , 345, 412.Google Scholar
Leibundgut, B. 1988, Ph.D. thesis, Universität Basel.Google Scholar
Nomoto, H. 1989, Exploring SN 1987A (in Japanese), (Tokyo: Kodansha).Google Scholar
Nomoto, K., Filippenko, A.V., and Shigeyama, T. 1990c, Astr. Ap. , in press.Google Scholar
Nomoto, K., and Hashimoto, M. 1988, Physics Reports , 163, 13.Google Scholar
Nomoto, K., and Kondo, Y. 1991, Ap. J. (Letters) , in press.Google Scholar
Nomoto, K., Shigeyama, T., and Hashimoto, M. 1988a, in IAU Colloquium 108, Atmospheric Diagnostics of Stellar Evolution , ed. Nomoto, K., Lecture Notes in Physics , 305, 319.Google Scholar
Nomoto, K., Shigeyama, T., Kumagai, S., and Hashimoto, M. 1988b, in Proc. Astr. Soc. Australia , 7, 490.Google Scholar
Nomoto, K., Shigeyama, T., Kumagai, S., and Yamaoka, H. 1990a, in Supernovae , ed. Woosley, S.E. (Springer-Verlag), in press.Google Scholar
Nomoto, K., Shigeyama, T., Yanagita, S., Hayakawa, S., and Yasuda, K. 1990b, in Chemical and Dynamical Evolution of Galaxies , eds. Ferrini, F., Franco, J., and Matteucci, F. (Pisa: Giondini), in press.Google Scholar
Nomoto, K., Thielemann, F.-K., and Yokoi, K. 1984, Ap. J. , 286, 644.Google Scholar
Panagia, N. 1987, in High Energy Phenomena Around Collapsed Stars , ed. Pacini, F. (D. Reidel), p. 33.Google Scholar
Porter, A.C., and Filippenko, A.V. 1987, Astr. J. 93, 1372 Google Scholar
Schaeffer, R., Casse, M., and Cahen, S. 1987, Ap. J. , 316, L31.Google Scholar
Schlegel, E.M., and Kirshner, R.P. 1989, A. J. , 98, 577.Google Scholar
Shigeyama, T., and Nomoto, K. 1990, Ap. J. , 360, 242.CrossRefGoogle Scholar
Shigeyama, T., Nomoto, K., and Hashimoto, M. 1988, Astr. Ap. , 196, 141.Google Scholar
Shigeyama, T., Nomoto, K., Tsujimoto, T., and Hashimoto, M. 1990, Ap. J. (Letters) , 361, L23.Google Scholar
Suntzeff, N.B., Hamuy, M., Martin, G., Gomez, A., and Gonzalez, R. 1988, A. J. , 96, 1864.Google Scholar
Swartz, D.A., Wheeler, J.C., and Harkness, R.P., 1990, Ap. J. , submitted.Google Scholar
Thielemann, F.-K., Hashimoto, M., and Nomoto, K. 1990, Ap. J. , 349, 222.CrossRefGoogle Scholar
Thielemann, F.-K., Nomoto, K., and Yokoi, K. 1986, Astr. Ap. , 158, 17.Google Scholar
Tornambe, A., and Matteucci, F. 1986, M. N. R. A. S. , 223, 69.CrossRefGoogle Scholar
Tsvetkov, D.Yu. 1985, Sov. Astr. , 29, 211.Google Scholar
Turatto, M., Cappellaro, E., Barbon, R., Delia Valle, M., Ortolani, S., and Rosino, L. 1990, A. J., in press.Google Scholar
Uomoto, A. 1986, Ap. J. (Letters) , 310, L35.Google Scholar
Uomoto, A., and Kirshner, R.P. 1985, Astr. Ap. , 149, L7.Google Scholar
Webbink, R. 1984, Ap. J. , 277, 355.Google Scholar
Wheeler, J.C., and Levreault, R. 1985, Ap. J. (Letters) , 294, L17.Google Scholar
Wheeler, J.C., and Harkness, R. 1990, Phys. Rep. , in press.Google Scholar
Whitelock, C. et al. 1989, M. N. R. A. S. , 240, 7p.Google Scholar
Witteborn, F.C., Bregman, J.D., Wooden, D.H., Pinto, P.A., Rank, D.M., Woosley, S.E., and Cohen, M. 1989, Ap. J. (Letters) , 338, L9.Google Scholar
Woosley, S.E. 1988, Ap. J., 330, 218.Google Scholar
Woosley, S.E., and Weaver, T.A. 1986, Ann. Rev. Astr. Ap. , 24, 205.CrossRefGoogle Scholar
Yamaoka, H., and Nomoto, K. 1990, in SN 1987A and Other Supernovae , ed. Danziger, I.J. (Garching: ESO), in press.Google Scholar
Yanagida, S., Nomoto, K., and Hayakawa, S. 1990, in Proceedings of the 21st International Cosmic Ray Conference (Adelaide) , 4, 44.Google Scholar