A very massive spectroscopic binary in the LH 54 OB association in the Large Magellanic Cloud

被引：8
|
作者：
Ostrov, PG [1 ]
机构：
[1] Fac Ciencias Astron & Geofis, RA-1900 La Plata, Argentina
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2002年 / 336卷 / 01期
关键词：
binaries : eclipsing; stars : early-type; stars : fundamental parameters; stars : individual : LH 54-425; Magellanic Clouds;
D O I：
10.1046/j.1365-8711.2002.05754.x
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We announce the discovery of a new early-type, double-lined spectroscopic binary in the LH 54 OB association in the Large Magellanic Cloud. We present a V light curve and radial velocities. We investigate the possible configurations of the system, concluding that it probably contains the most massive star measured at the present, with a mass of the order of 100 M., while its companion has approximately 50 M..
引用
收藏
页码：309 / 314
页数：6
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