A PERIOD-LUMINOSITY RELATION FOR SUPER-GIANT RED VARIABLES IN THE LARGE MAGELLANIC CLOUD

被引：39
|
作者：
FEAST, MW
CATCHPOLE, RM
CARTER, BS
ROBERTS, G
机构：
[1] South African Astronomical Observatory, PO Box 9, Observatory,7935, South Africa
来源：
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1980年 / 193卷 / 02期
关键词：
D O I：
10.1093/mnras/193.2.377
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Infrared photometry for 24 red supergiant variables in the LMC is used to derive bolometric magnitudes. The existence of a period-luminosity relation for these stars is demonstrated and compared with theory. © Royal Astronomical Society.
引用
收藏
页码：377 / 380
页数：4
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