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- W2166847215 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 () 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." @default.
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- W2166847215 date "2008-03-11" @default.
- W2166847215 modified "2023-09-25" @default.
- W2166847215 title "Improved orbital solution and masses for the very low-mass multiple system LHS 1070" @default.
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- W2166847215 doi "https://doi.org/10.1051/0004-6361:20078875" @default.
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