THE OLD GALACTIC CLUSTER NGC-188 AND THE ORIGIN OF THE W-URSAE MAJORIS TYPE CONTACT BINARIES

被引：17

作者：

BALIUNAS, SL ^{[1
]}

GUINAN, EF ^{[1
]}

机构：

[1] VILLANOVA UNIV,DEPT ASTRON,VILLANOVA,PA 19085

来源：

ASTROPHYSICAL JOURNAL | 1985年 / 294卷 / 01期

关键词：

D O I：

10.1086/163288

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：207 / 215

页数：9

共 71 条

[1]

ARTUIKHINA NM, 1964, PEREM ZVEZDY, V15, P127

[2]

Baliunas S. L., 1984, Cool Stars, Stellar Systems and the Sun. Proceedings of the Third Cambridge Workshop, P223

[3]

BALIUNAS SL, 1983, B AAS, V15, P924

[4]

BINNENDIJK L, 1965, 3D IAU C VAR STARS P, V40, P36

[5]

BINNENDIJK L, 1970, VISTAS ASTRON, V12, P211

[6]

BINNENDIJK L, 1960, PROPERTIES DOUBLE ST, P148

[7]

Bopp B. W., 1981, IAU S, V93, P177

[8]

Budding E., 1982, Binary and Multiple Stars as Tracers of Stellar Evolution. Proceedings of the 69th Colloquium of the International Astronomical Union, P351

[9] CONTACT BINARY STARS .1. AN X-RAY SURVEY [J].

CRUDDACE, RG ;

DUPREE, AK .

ASTROPHYSICAL JOURNAL, 1984, 277 (01) :263-273

[10]

DORREN JD, 1984, BAAS, V16, P474

← 1 2 3 4 5 6 7 8 →