A MODEL OF THE CYGNUS LOOP

被引：40

作者：

FALLE, SAEG

GARLICK, AR

机构：

[1] School of Mathematics, The University, Leeds,LS2 9JT, United Kingdom

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1982年 / 201卷 / 02期

关键词：

D O I：

10.1093/mnras/201.3.635

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a model of the Cygnus Loop based on a supernova exploding into a region of the interstellar medium containing a density discontinuity. The breakout phenomenon is then able to explain the high velocity optical emission observed in this remnant by Kirschner & Taylor (1976). It also gives rise to two X-ray emitting components whose intensity and hardness variations over the remnant are in agreement with observations. © 1982 Royal Astronomical Society.

引用

页码：635 / 644

页数：10

共 19 条

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