The double-lined spectroscopic binary haro 1-14c

被引:0
作者
Prato, L [1 ]
Simon, M [1 ]
机构
[1] Lowell Observ, Flagstaff, AZ 86001 USA
来源
Astrometry in the Age of the Next Generation of Large Telescopes | 2005年 / 338卷
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中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report detection of the low-mass secondary in the spectroscopic binary Haro 1-14c in the Ophiuchus star forming region. The secondary/primary mass ratio is 0.310 +/- 0.014. With an estimated photometric primary mass of 1.2 M-circle dot, the secondary mass is similar to 0.4 M-circle dot and the projected semi-major axis is similar to 1.5 AU. The system is well-suited for astrometric mapping of its orbit with the current generation of ground-based IR interferometers. This could yield precision values of the system's component masses and distance.
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页码:284 / 287
页数:4
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