Continuum emission from classical nova winds
Continuum emission from classical nova winds
复制标题
经典新星风的连续发射
DOI：
10.1093/mnras/204.1.45
复制
发表时间：
1983
影响因子：
4.8
通讯作者：
R. Harkness
中科院分区：
文献类型：
--
作者：
R. Harkness
在准定常光学厚度跨音速风模式中，考虑了爆发过程中缓慢的经典新星的涌现连续体。给出了各种稳定质量损失率的模型，并与下降期间和峰值后早期的慢新星的演化有关。连续发射被发现从根本上偏离了黑体光谱，并显示出高度延伸的恒星大气的共同特征。
The emergent continuum of a slow classical nova during outburst is considered in the quasi-steady optically thick, transsonic wind model of Ruggles & Bath. Models are presented for various steady mass loss rates and are related to the evolution of slow novae during decline and early post-maximum. The continuum emission is found to depart radically from a blackbody spectrum and to exhibit features common to highly extended stellar atmospheres.