GRAVITATIONAL-RADIATION AND THE EVOLUTION OF CATACLYSMIC BINARIES

被引：35

作者：

TAAM, RE

FLANNERY, BP

FAULKNER, J

机构：

[1] HARVARD UNIV,SMITHSONIAN CTR ASTROPHYS,CAMBRIDGE,MA 02138

[2] UNIV CALIF SANTA CRUZ,LICK OBSERV,BOARD STUDIES ASTRON & ASTROPHYS,SANTA CRUZ,CA 95064

来源：

ASTROPHYSICAL JOURNAL | 1980年 / 239卷 / 03期

关键词：

D O I：

10.1086/158190

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：1017 / 1023

页数：7

共 19 条

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[5] ULTRASHORT-PERIOD BINARIES II HZ 29 (=AM CVN) - DOUBLE-WHITE-DWARF SEMIDETACHED POSTCATACLYSMIC NOVA [J].

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FLANNERY, BP ;

WARNER, B .

ASTROPHYSICAL JOURNAL, 1972, 175 (02) :L79-&

[6] ULTRASHORT-PERIOD BINARIES, GRAVITATIONAL RADIATION, AND MASS TRANSFER .1. STANDARD MODEL, WITH APPLICATIONS TO WZ SAGITTAE AND Z CAMELOPARDALIS [J].

FAULKNER, J .

ASTROPHYSICAL JOURNAL, 1971, 170 (03) :L99-&

[7]

FAULKNER J, 1976, STRUCTURE EVOLUTION, P193

[8] ORIGIN OF CENTAURUS X-3 AND RELATED BINARY X-RAY SOURCES [J].

FLANNERY, BP ;

ULRICH, RK .

ASTROPHYSICAL JOURNAL, 1977, 212 (02) :533-540

[9]

FLANNERY BP, 1978, ANN NY ACAD SCI, V302, P36

[10]

GIANNONE P, 1970, ASTRON ASTROPHYS, V4, P428

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