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On the Physical Model of Supernovae Close to Light Maximum

Published online by Cambridge University Press:  30 March 2016

E. R. Mustel
E. R. Mustel*
Affiliation:
Astronomical Council, USSR Academy of Sciences, Moscow, U.S.S.R.

Abstract

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One of the principal sources of information about supernovae are the spectra of these stars. Thus we are going to discuss mainly the spectra of type I and type II supernovae around light maximum (tmax).

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 3: Highlights of Astronomy. As presented at the XVth General Assembly of the IAU, 1973 , 1974 , pp. 545 - 557
Copyright
Copyright © Reidel 1974

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