NUMERICAL COMPUTATION OF DYNAMICAL EVOLUTION OF A SUPERNOVA REMNANT

被引：60

作者：

ROSENBERG, I ^{[1
]}

SCHEUER, PAG ^{[1
]}

机构：

[1] MULLARD RADIO ASTRON OBSERV, CAMBRIDGE, ENGLAND

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1973年 / 161卷 / 01期

关键词：

Astrophysics; -; NASA;

D O I：

10.1093/mnras/161.1.27

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

This paper presents a numerical computation of the dynamical development of a simple model of a supernova remnant in which an expanding shell of ejected matter interacts with the interstellar gas. The evolution is followed continuously through the stages approximating to an undecelerated expansion, adiabatic blast wave and the stage dominated by radiative cooling. © 1973 Royal Astronomical Society. Provided by the NASA Astrophysics Data System.

引用

页码：27 / 45

页数：19

共 30 条

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