INDICATION OF THE HIGH MASS-TRANSFER RATIO IN S-TYPE SYMBIOTIC BINARIES

被引：0
|
作者：
Shagatova, N. [1 ]
Skopal, A. [1 ]
机构：
[1] Slovak Acad Sci, Astron Inst, Tatranska Lomnica, Slovakia
来源：
PHYSICS OF EVOLVED STARS: A CONFERENCE DEDICATED TO THE MEMORY OF OLIVIER CHESNEAU | 2015年 / 71-72卷
关键词：
RADIO SURVEY; STARS;
D O I：
10.1051/eas/1571044
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
By modelling H-0 column densities in eclipsing S-type symbiotic stars EG And and SY Mus, we derived the wind velocity profile and the corresponding mass-loss rate from their giants. Our analysis revealed a strong enhancement of the wind at the orbital plane.
引用
收藏
页码：195 / 196
页数：2
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