THE LUMINOSITY CORE MASS RELATION - WHY AND HOW

被引：20

作者：

TUCHMAN, Y

GLASNER, A

BARKAT, Z

机构：

来源：

ASTROPHYSICAL JOURNAL | 1983年 / 268卷 / 01期

关键词：

D O I：

10.1086/160958

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：356 / 360

页数：5

共 15 条

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[7] THERMAL PULSE AND INTERPULSE PROPERTIES OF INTERMEDIATE-MASS STELLAR MODELS WITH CARBON-OXYGEN CORES OF MASS 0.96, 1.16, AND 1.36M. [J].

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[10]

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