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| Paper: |
The Double-Lined Spectroscopic Binary Haro 1-14c |
| Volume: |
338, Astrometry in the Age of the Next Generation of Large Telescopes |
| Page: |
284 |
| Authors: |
Prato, L.; Simon, M. |
| Abstract: |
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 MSolar, the secondary mass is ~ 0.4 MSolar and the projected semi-major axis is ~ 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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