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

页码：155 / 157

页数：3