MIRA LIGHT CURVES AND MASS-LOSS

被引：1
|
作者：
ALARD, C
机构：
来源：
ASTROPHYSICS AND SPACE SCIENCE | 1994年 / 217卷 / 1-2期
关键词：
LPVS; LIGHT CURVES; MASS LOSS;
D O I：
10.1007/BF00990047
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Long Period Variables represent a late stage in the evolution of intermediate mass stars. Mass loss wich leads them to planetary nebulae within a few 10(5) years, is a complex process and the object of many investigations. Recents studies suggest that mass loss could occur in brief superwind phases separated by long quiescent periods. Here we produce a total of about one hundred light curves of Mira stars. Furthermore some relationships between mass loss and the shape of the light curve are analysed in this article.
引用
收藏
页码：155 / 157
页数：3
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