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：

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

[11] A STUDY OF SOLAR EVOLUTION [J].

EZER, D ;

CAMERON, AGW .

[12] THERMONUCLEAR REACTION RATES [J].

FOWLER, WA ;

CAUGHLAN, GR ;

ZIMMERMAN, BA .

[13] STELLAR EVOLUTION .I. APPROACH TO MAIN SEQUENCE [J].

IBEN, I .

[14]

IBEN I, 1965, ASTROPHYS J, V142, P1147

[15]

Paczynski B., 1970, Acta Astronomica, V20, P47

[16] N14(ALPHA,GAMMA)F18 REACTION [J].

PARKER, PD .

PHYSICAL REVIEW, 1968, 173 (04) :1021-+

[17]

REEVES H, 1965, STARS STELLAR SYSTEM, V8

[18] ELECTRON SCREENING AND THERMONUCLEAR REACTIONS [J].

SALPETER, EE .

AUSTRALIAN JOURNAL OF PHYSICS, 1954, 7 (03) :373-388