THEORETICAL EVOLUTION OF A HYDROGEN-HELIUM STAR OF 3M FROM PRE-MAIN SEQUENCE TO CORE HELIUM-EXHAUSTION PHASE

被引：16

作者：

EZER, D

机构：

[1] NASA,GODDARD INST SPACE STUDIES,NEW YORK,NY 10025

[2] YESHIVA UNIV,BELFER GRAD SCH SCI,NEW YORK,NY 10033

来源：

ASTROPHYSICS AND SPACE SCIENCE | 1972年 / 18卷 / 01期

关键词：

D O I：

10.1007/BF00645294

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：226 / 245

页数：20

共 18 条

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[4]

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[5]

Bohm-Vitense E., 1958, Z ASTROPHYS, V46, P108

[6]

CAMERON AGW, 1971, ASTROPHYS SPACE SCI, V16, P179

[7]

CAUCH R, 1972, ASTROPHYS J, V172, P395

[8] EVOLUTION OF HYDROGEN-HELIUM STARS [J].

EZER, D ;

CAMERON, AGW .

ASTROPHYSICS AND SPACE SCIENCE, 1971, 14 (02) :399-&

[9] EARLY AND MAIN SEQUENCE EVOLUTION OF STARS IN RANGE 0.5 TO 100 SOLAR MASSES [J].

EZER, D ;

CAMERON, AGW .

CANADIAN JOURNAL OF PHYSICS, 1967, 45 (11) :3429-&

[10] PRE-MAIN SEQUENCE STELLAR EVOLUTION WITH MASS LOSS [J].

EZER, D ;

CAMERON, AGW .

ASTROPHYSICS AND SPACE SCIENCE, 1971, 10 (01) :52-&

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