A THEORY FOR GAMMA-RAY AND X-RAY BURST SOURCES

被引：0
|
作者：
BROWNE, PF
机构：
[1] Physics Department, UMIST, Manchester
来源：
ASTROPHYSICS AND SPACE SCIENCE | 1995年 / 231卷 / 1-2期
关键词：
D O I：
10.1007/BF00658664
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A common mechanism for both X-ray and gamma-ray bursters is proposed on the basis that a ''window'' can be created transiently in the polar cap of a degenerate star, a white dwarf for X-ray bursts and a neutron star for gamma-ray bursts. The ''window'' exposes transiently a hot degenerate sub-layer of the star at shallow depth, from which escapes blackbody flux for a source at temperature 3 kev with window radius 10 km in the case of X-ray bursts and for a source at temperature 300 kev with window radius 0.5 km in the case of gamma-ray bursts.
引用
收藏
页码：431 / 436
页数：6
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