POSSIBILITY OF MAGNETIC STARSPOTS ON PRIMARY COMPONENTS OF W-URSAE MAJORIS TYPE BINARIES

被引：106

作者：

MULLAN, DJ ^{[1
]}

机构：

[1] FRANKLIN INST,BARTOL RES FDN,SWARTHMORE,PA 19081

来源：

关键词：

D O I：

10.1086/153635

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：563 / 573

页数：11

共 61 条

[1]

AMBROZ P, 1971, SOLAR MAGNETIC FIELD, P696

[2]

BAKER NH, 1966, TABLES CONVECTIVE ST, P21

[3]

BERGEAT J, 1972, ASTRON ASTROPHYS, V17, P215

[4]

BERNACCA PL, 1974, ASTRON ASTROPHYS, V33, P443

[5] LIGHT VARIATION AND ORBITAL ELEMENTS OF AM LEONIS [J].

BINNENDIJK, L .

[6]

BINNENDIJK L, 1974, COMMUNICATION

[7]

Binnendijk L., 1970, VISTAS ASTRON, V12, P217, DOI DOI 10.1016/0083-6656(70)90041-3

BOPP, BW ;

EVANS, DS .

[9]

BUMBA V, 1973, B ASTRON I CZECH, V24, P22

[10] PERIODICITIES IN SOLAR-ACTIVITY [J].

COLE, TW .