We present radial velocities of the M8V-type, very low-mass star vB 10 that have been obtained at four different epochs of observations 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, a result that is consistent with the recent finding of a massive planet companion around the star by Pravdo & Shaklan (2009). 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.
@article{arxiv.0908.3751,
title = {Infrared radial velocities of vB 10},
author = {M. R. Zapatero Osorio and E. L. Martin and C. del Burgo and R. Deshpande and M. M. Montgomery},
journal= {arXiv preprint arXiv:0908.3751},
year = {2015}
}