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arXiv · 0803.0628

Improved orbital solution and masses for the very low-mass multiple system LHS 1070

A. Seifahrt·T. Roell·R. Neuhaeuser·A. Reiners·F. Kerber·H. U. Kaeufl·R. Siebenmorgen·A. Smette
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Abstract

We present a refined orbital solution for the components A, B, and C of the nearby late-M type multiple system LHS 1070. By combining astrometric datapoints from NACO/VLT, CIAO/SUBARU, and PUEO/CFHT, as well as a radial velocity measurement from the newly commissioned near infrared high-resolution spectrograph CRIRES/VLT, we achieve a very precise orbital solution for the B and C components and a first realistic constraint on the much longer orbit of the A-BC system. Both orbits appear to be co-planar. Masses for the B and C components calculated from the new orbital solution (M_(B+C) = 0.157 +/- 0.009 M_sun) are in excellent agreement with theoretical models, but do not match empirical mass-luminosity tracks. The preliminary orbit of the A-BC system reveals no mass excess for the A component, giving no indication for a previously proposed fourth (D) component in LHS 1070.

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A. Seifahrt, T. Roell, R. Neuhaeuser, A. Reiners, F. Kerber, H. U. Kaeufl, R. Siebenmorgen, A. Smette. 2008-03-05. Improved orbital solution and masses for the very low-mass multiple system LHS 1070. https://doi.org/10.1051/0004-6361:20078875

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