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
收藏
页码：299 / 301
页数：3
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