Infrared radial velocities of vB 10

Carlos Del Burgo, DEE Group Author

Research output: Contribution to journalArticlepeer-review


We present radial velocities of the M8V-type, very low-mass star vB 10 obtained at four different epochs between 2001 and 2008. We use high-resolution (R ~ 20 000) near-infrared (J-band) spectra taken with the NIRSPEC instrument on the Keck II telescope. Our data suggest that vB 10 shows radial velocity variability with an amplitude of ~1 km s-1, a result that is consistent with the recent finding of a massive planet companion around the star. More velocity measurements and a better sampling of the orbital phase are required to precisely constrain the orbital parameters and the individual masses of the pair.
Original languageUnknown
Pages (from-to)L5-L8
JournalAstronomy and Astrophysics
Issue number1
Publication statusPublished - 1 Jan 2009

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