AN ASTROMETRIC STUDY OF 4 BINARY STARS

被引：18

作者：

HEINTZ, WD ^{[1
]}

CANTOR, BA ^{[1
]}

机构：

[1] WIDENER UNIV,DEPT PHYS,CHESTER,PA 19013

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC | 1994年 / 106卷 / 698期

关键词：

D O I：

10.1086/133386

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Completion of long-term astrometric plate series yields revised results on the orbits and parallaxes. The subdwarf mu Cassiopeiae seems to be overluminous; the distance of the supergiant epsilon Aurigae is near 600 pc. The unresolved companion in the red dwarf pair BD +6398-degrees is of very low mass, and the companion of BD +67552-degrees massive but probably underluminous.

引用

页码：363 / 364

页数：2

共 13 条

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