Optical, infrared, and bolometric light curves of type Ia supernovae

被引：14

作者：

Suntzeff, NB ^{[1
]}

机构：

[1] Natl Opt Astron Observ, Cerro Tololo Inter Amer Observ, La Serena, Chile

来源：

FROM TWILIGHT TO HIGHLIGHT: THE PHYSICS OF SUPERNOVAE | 2003年

关键词：

D O I：

10.1007/10828549_24

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The thermalized energy from the radioactive decays of Ni-56 and Ni-57 and their daughter nuclides power the light curves of supernovae near maximum light. The bolometric light curve gives us a fundamental understanding of the energy evolution of a supernova explosion and the amount of radioactive nuclides produced. In this review, I will, discuss the bolometric evolution of the Type IIp supernovae SN1987A, and the general class of bolometric light curves of Type la thermonuclear explosions.

引用

页码：183 / 192

页数：10

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