Classical nova models with accretion heating at accretion rates of 10 exp -9 and 10 exp - 10 solar masses per year
Classical nova models with accretion heating at accretion rates of 10 exp -9 and 10 exp - 10 solar masses per year
复制标题
具有每年 10 exp -9 和 10 exp - 10 个太阳质量的吸积加热的经典新星模型
DOI：
10.1086/170972
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发表时间：
1992
期刊：
影响因子：
--
通讯作者：
A. Kovetz
中科院分区：
文献类型：
--
作者：
D. Prialnik;A. Kovetz
计算了M=10 −10 M yr −1和M=10 −9 M yr −1的1.25 M C-O白色矮星上吸积的两个演化序列，它们经历了热核逃逸和质量损失的动力学阶段，然后是残余物的收缩和衰退。改进的算法被用于在吸积阶段的扩散和质量损失的计算。考虑了增积加热
Two evolutionary sequences of accretion onto a 1.25 M ⊙ C-O white dwarf are computed for M=10 −10 M ⊙ yr −1 and M=10 −9 M ⊙ yr −1 and are carried through the thermonuclear runaway and the dynamical phases of mass loss, followed by contraction of the remnant and decline. Improved algorithms are used for diffusion during the accretion phase and for the computation of mass loss. Accretional heating is taken into account