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
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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.
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页码:168 / 169
页数:2
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