HARD EMISSION FROM CLASSICAL NOVAE

被引：0
|
作者：
LEISING, MD
机构：
来源：
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1993年 / 97卷 / 01期
关键词：
NUCLEOSYNTHESIS; NOVAE; GAMMA-RAYS; THEORY; X-RAYS; STARS;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The thermonuclear model of classical novae has been very successful in explaining many observed features of novae. It also predicts unique gamma-ray and X-ray signatures, a few of which possibly have already been observed. We describe recent developments in the expectations of these signatures and we discuss prospects for additional observations with current observatories.
引用
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页码：299 / 301
页数：3
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