RECENT PROGRESS IN UNDERSTANDING THE ERUPTIONS OF CLASSICAL NOVAE
RECENT PROGRESS IN UNDERSTANDING THE ERUPTIONS OF CLASSICAL NOVAE
复制标题
了解经典新星爆发的最新进展
DOI：
10.1086/132400
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发表时间：
1989
影响因子：
3.5
通讯作者：
M. Shara
中科院分区：
文献类型：
--
作者：
M. Shara
回顾了产生新星喷发的物理过程，以及二元系统参数（例如白矮星的化学成分或质量以及质量吸积率）对新星喷发的影响。还考虑了从矮星到经典新星并再次变回的可能变态、新星的 X 射线和伽马射线发射、以及球状星团和河外系统中新星的特征和分布。讨论了热核失控模型的局限性。
The physical processes generating nova eruptions are reviewed, along with the effects on nova eruptions of binary-system parameters such as the chemical composition or mass of the white dwarf and the mass accretion rate. Also considered are the possible metamorphosis from dwarf to classical novae and back again, X-ray and gamma-ray emission from novae, and the characteristics and distributions of novae in globular clusters and extragalactic systems. Limitations of the thermonuclear runaway model are discussed.