CLOSE BINARY-SYSTEMS BEFORE AND AFTER MASS-TRANSFER .2. SEMI-DETACHED SYSTEMS

被引：11

作者：

DEGREVE, JP

机构：

来源：

ASTROPHYSICS AND SPACE SCIENCE | 1980年 / 72卷 / 02期

关键词：

D O I：

10.1007/BF00639147

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：411 / 432

页数：22

共 47 条

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[Anonymous], ACA

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[6] EVOLUTION OF MASSIVE CLOSE BINARIES .6. FINAL CONSIDERATIONS FOR CONSERVATIVE CASE [J].

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VANDESSEL, EL .

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[7]

Delgado A., 1979, International Astronomical Union Symposium. No.83. Mass Loss and Evolution of O-Type Stars, P415

[8] EVOLUTION OF ROTATING STARS .3. PREDICTED SURFACE ROTATION VELOCITIES FOR STARS WHICH CONSERVE TOTAL ANGULAR-MOMENTUM [J].

ENDAL, AS ;

SOFIA, S .

ASTROPHYSICAL JOURNAL, 1979, 232 (02) :531-540

[9] ABSOLUTE DIMENSIONS OF 140 CLOSE BINARY-SYSTEMS [J].

GIANNONE, P ;

GIANNUZZI, MA .

ASTROPHYSICS AND SPACE SCIENCE, 1974, 26 (02) :289-304

[10]

HORN J, 1971, B ASTRON I CZECH, V22, P37

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