A Spectroscopic Binary at the M/L Transition
Abstract
We report the discovery of a single-lined spectroscopic binary with an Ultra Cool Dwarf (UCD) primary with a spectral type between M8 and L0.5. This system was discovered during the course of an ongoing survey to monitor L dwarfs for radial velocity variations and is the first known small separation (a<1 AU) spectroscopic binary among dwarfs at the M/L transition. Based on radial-velocity measurements with a typical precision of 300 m/s we estimate the orbital parameters of this system to be P=246.73+/-0.49 d, a1 sin(i)=0.159+/-0.003 AU, M2 sin(i)=0.2062 (M1+M2)^(2/3)+/-0.0034 M_{\sun}. Assuming a primary mass of M1=0.08M_{\sun} (based on spectral type), we estimate the secondary minimum mass to be M2 sin(i)=0.054 M_{\sun}. With future photometric, spectroscopic, and interferometric observations it may be possible to determine the dynamical masses of both components directly, making this system one of the best characterized UCD binaries known.
Cite
@article{arxiv.0804.1364,
title = {A Spectroscopic Binary at the M/L Transition},
author = {Cullen H. Blake and David Charbonneau and Russel J. White and Guillermo Torres and Mark S. Marley and Didier Saumon},
journal= {arXiv preprint arXiv:0804.1364},
year = {2009}
}
Comments
11 pages, 2 figures. Accepted for publication in ApJ Letters