EVOLUTION OF MASSIVE CLOSE BINARIES .5. SYSTEMS CONTAINING PRIMARIES WITH MASSES BETWEEN 10-M AND 15-M

被引：22

作者：

DEGREVE, JP ^{[1
]}

DELOORE, C ^{[1
]}

机构：

[1] VRIJE UNIV BRUSSEL,B-1050 BRUSSELS,BELGIUM

来源：

ASTROPHYSICS AND SPACE SCIENCE | 1977年 / 50卷 / 01期

关键词：

D O I：

10.1007/BF00648520

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：75 / 85

页数：11

共 22 条

[1]

Arnett W. D., 1973, EXPLOSIVE NUCLEOSYNT, P236

[2]

COX JP, 1968, STELLAR STRUCTURE, P891

[3] EVOLUTION OF MASSIVE CLOSE BINARIES .4. EVOLUTION OF A 10M.+8M. SYSTEM INTO A SYSTEM WITH A WHITE-DWARF COMPONENT [J].

DEGREVE, JP ;

DELOORE, C .

ASTROPHYSICS AND SPACE SCIENCE, 1976, 43 (01) :35-46

[4] EVOLUTION OF MASSIVE CLOSE BINARIES .3. POSSIBILITY OF A TIDAL INSTABILITY DURING POST SUPERNOVA PHASE [J].

DEGREVE, JP ;

DELOORE, C ;

SUTANTYO, W .

ASTROPHYSICS AND SPACE SCIENCE, 1975, 38 (02) :301-312

[5]

DEGREVE JP, 1976, THESIS VRIJE U

[6] EVOLUTION OF MASSIVE CLOSE BINARIES .1. X-RAY BINARY STAGE [J].

DELOORE, C ;

DEGREVE, JP .

ASTROPHYSICS AND SPACE SCIENCE, 1975, 35 (02) :241-247

[7]

DELOORE C, 1975, 1974 P IAU REG M TRI

[8]

DELOORE C, 1976, STRUCTURE EVOLUTION, V73, P27

[9] THEORETICAL STUDIES OF MASSIVE STARS .1. EVOLUTION OF A 15M PERIOD STAR FROM ZERO-AGE MAIN-SEQUENCE TO NEON IGNITION [J].

ENDAL, AS .

ASTROPHYSICAL JOURNAL, 1975, 197 (02) :405-413

[10]

ENDAL AS, 1974, THESIS U FLORIDA

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