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Recent Optical Observations of Supernovae

Published online by Cambridge University Press:  30 March 2016

Alexei V. Filippenko
Alexei V. Filippenko*
Affiliation:
Department of Astronomy University of CaliforniaBerkeley, CA 94720 USA

Abstract

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This paper reviews some of the basic optical properties of supernovae (SNe), concentrating on the most interesting new observations. It is emphasized that SNe can be securely subdivided into the two well-known classes (Type I and Type II) only on the basis of their spectra, since the light curves alone can be misleading. Brief interpretations of the spectra and light curves are presented. Spectroscopic and photometric characteristics of “peculiar” Type I supernovae (SNe I-pec), which may be physically distinct from “normal” SNe I, are discussed. Finally, the complete optical spectrum of SN 1985f in NGC 4618 is illustrated, and comparisons are made with the spectra of SNe I and SNe II. No resemblance is found, suggesting that this object belongs to a truly new class (Type III) of SNe. There is, however, very recent evidence that the spectra of SNe I-pec obtained more than eight months past maximum brightness are strikingly similar to that of SN 1985f.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 7: Highlights of Astronomy. As presented at the XIXth General Assembly of the IAU, 1985 , 1986 , pp. 589 - 598
Copyright
Copyright © Reidel 1986

References

Axelrod, T. S. 1980, in Type I Supernovae, ed. Wheeler, J. C. (Austin: University of Texas), p. 80.Google Scholar
Balick, B., and Heckman, T. 1978, Ap. J. (Letters), 226, L7.CrossRefGoogle Scholar
Barbon, R. 1978, Mem. Soc. Ast. It., 49, 331.Google Scholar
Barbon, R., Ciatti, F., and Rosino, L. 1973, Astr. Ap., 25, 241.Google Scholar
Barbon, R., Ciatti, F., and Rosino, L. 1979, Astr. Ap., 72, 287.Google Scholar
Begelman, M. C., and Sarazin, C. L. 1986, Ap. J. (Letters), in press.Google Scholar
Bertola, F. 1964, Ann. d’Ap., 27, 319.Google Scholar
Bertola, F., Mammano, A., and Perinotto, M. 1965, Contr. Asiago Obs., No. 174.Google Scholar
Blair, W. P., Kirshner, R. P., and Winkler, P. F. Jr. 1983, Ap. J., 272, 84.Google Scholar
Branch, D. 1982, in Supernovae: A Survey of Current Research, eds. Rees, M. J. and Stoneham, R. J. (Dordrecht: Reidel), p. 267.Google Scholar
Branch, D., Falk, S. W., McCall, M. L., Rybski, P., Uomoto, A. K., and Wills, B. J. 1981, Ap. J., 244, 780.Google Scholar
Branch, D., Lacy, C. H., McCall, M. L., Sutherland, P. G., Uomoto, A., Wheeler, J. C., and Wills, B. J. 1983, Ap. J., 270, 123.CrossRefGoogle Scholar
Cahen, S., Schaeffer, R., and Cassé, M. 1986, in Fifth Moriond Astrophysics Meeting: Nucleosynthesis and its Implications on Nuclear and Particle Physics, ed. Audouze, J. (Dordrecht: Reidel).Google Scholar
Chevalier, R. A. 1976, Ap. J., 208, 826.Google Scholar
Chevalier, R. A. 1986, Highlights of Astronomy, this volume.Google Scholar
De Robertis, M. M., and Pinto, P. A. 1985, Ap. J. Letters, 293, L77.Google Scholar
Doggett, J. B., and Branch, D. 1985, A. J., 90, 2303 (DB85).CrossRefGoogle Scholar
Elias, J. H., Matthews, K., Neugebauer, G., and Persson, S. E. 1985, Ap. J., 296, 379.Google Scholar
Filippenko, A. V., and Sargent, W. L. W. 1985, Nature, 316, 407.Google Scholar
Filippenko, A. V., and Sargent, W. L. W. 1986a, A. J., in press (April issue).Google Scholar
Filippenko, A. V., and Sargent, W. L. W. 1986b, in preparation.Google Scholar
Gaskell, C. M., Cappellaro, E., Dinerstein, H., Garnett, D., Harkness, R. P., and Wheeler, J. C. 1986, Ap. J. (Letters), in press.Google Scholar
Goss, W. M., Ekers, R. D., Danziger, I. J., and Israel, F. P. 1980, M. N. R. A. S., 193, 901.Google Scholar
Greenstein, J., and Minkowski, R. 1973, Ap. J., 182, 225.CrossRefGoogle Scholar
Kirshner, R. P. 1985, private communication.Google Scholar
Kirshner, R. P., and Blair, W. P. 1980, Ap. J., 236, 135.Google Scholar
Kirshner, R. P., and Chevalier, R. A. 1977, Ap. J., 218, 142.Google Scholar
Kirshner, R. P., and Kwan, J. 1974, Ap. J., 193, 27.Google Scholar
Kirshner, R. P., and Kwan, J. 1975, Ap. J., 197, 415.Google Scholar
Kirshner, R. P., Oke, J. B., Pension, M. V., and Searle, L. 1973, Ap. J., 185, 303.Google Scholar
Lasker, B. M. 1978, Ap. J., 223, 109.Google Scholar
Litvinova, I. Yu., and Nadyozhin, D. K. 1983, Ap. Space Sci., 89, 89.Google Scholar
Minkowski, R. 1939, Ap. J., 89, 156.CrossRefGoogle Scholar
Niemela, V. S., Ruíz, M. T., and Phillips, M. M. 1985, Ap. J., 289, 52.CrossRefGoogle Scholar
Oke, J. B., and Searle, L. 1974, Ann. Rev. Astr. Ap., 12, 315.Google Scholar
Panagia, N. 1986, in High Energy Phenomena Around Collapsed Stars (Cambridge: Cambridge University Press), in press.Google Scholar
Porter, A. C. 1983, Bull. Amer. Astr. Soc., 15, 966.Google Scholar
Schurmann, S. R., Arnett, W. D., and Falk, S. W. 1979, Ap. J., 230, 11.Google Scholar
Uomoto, A., and Kirshner, R. P. 1985, Astr. Ap., 149, L7.Google Scholar
Wheeler, J. C., and Levreault, R. 1985, Ap. J. (Letters), 294, L17.Google Scholar
Zwicky, F. 1965, in Stars and Stellar Systems, Vol. 8, eds. Aller, L. H. and McLaughlin, D. B. (Chicago: University of Chicago Press), p. 367.Google Scholar