Rotational velocities of S-type symbiotic stars

被引：0
作者：
Fekel, RC [1 ]
Hinkle, KH
Joyce, RR
机构：
[1] Tennessee State Univ, Ctr Excellence Informat Syst, Nashville, TN 37203 USA
[2] Natl Opt Astron Observ, Tucson, AZ 85726 USA
来源：
STELLAR ROTATION | 2004年 / 215期
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We obtained high-resolution spectroscopic observations at 2.226 mum of 13 S-type symbiotic binaries using the Phoenix infrared spectrograph on Kitt Peak telescopes. From an empirical calibration we determined v sin i values for the giant components. Combined with information from a program to determine orbits, the rotational velocities have been used to estimate the sizes of these stars and the fraction of their Roche lobes that they fill.
引用
收藏
页码：168 / 169
页数：2
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