GAMMA-PERSEI - NOT OVERMASSIVE BUT OVERLUMINOUS

被引：22

作者：

POPPER, DM ^{[1
]}

MCALISTER, HA ^{[1
]}

机构：

[1] GEORGIA STATE UNIV,CTR HIGH ANGULAR RESOLUT ASTRON,ATLANTA,GA 30303

来源：

关键词：

D O I：

10.1086/114507

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：700 / 711

页数：12

共 36 条

[1]

BAHNG JDR, 1958, ASTROPHYS J, V128, P586

[2]

BALEGA YY, 1985, SOV ASTRON LETT+, V11, P47

[3]

BALEGA YY, 1984, ASTRON ASTROPHYS S, V58, P729

[4]

BLAZIT A, 1977, ASTROPHYS J LETT, V194, pL147

[5]

Bonneau D., 1984, Astronomy & Astrophysics Supplement Series, V58, P729

[6]

BONNEAU D, 1985, A AS, V65, P27

[7]

CAMPBELL WW, 1928, PUBL LICK OBS, V16

[8] SPECTRAL CLASSIFICATION OF BRIGHT F STARS [J].

COWLEY, AP .

[9]

Dudinov V. N., 1982, Instrumentation for Astronomy with Large Optical Telescopes. Proceedings of IAU Colloquium. No.67, P191

[10] BINARY STARS UNRESOLVED BY SPECKLE INTERFEROMETRY .3. [J].

HARTKOPF, WI ;

MCALISTER, HA .