A Possible Brown Dwarf Companion to the White Dwarf GD1400
Abstract
An unresolved, likely L dwarf companion to the DA white dwarf GD1400 is reported. This would be only the second such system known, discovered 17 years after the prototype L dwarf, GD165B, was determined to be a companion to a white dwarf. Photometric observations and model predicted stellar parameters of the well studied white dwarf primary indicate that GD1400B has and mag. If correct, this would place GD1400B at spectral type L6, and it would be the lowest luminosity unevolved companion known to a white dwarf, and thus a definite brown dwarf. However, a low resolution Keck NIRSPEC m spectrum may not be consistent with known L dwarfs. Uncertainties in classification remain until the binary is resolved or a trigonometric parallax is measured.
Keywords
Cite
@article{arxiv.astro-ph/0407036,
title = {A Possible Brown Dwarf Companion to the White Dwarf GD1400},
author = {J. Farihi and M. Christopher},
journal= {arXiv preprint arXiv:astro-ph/0407036},
year = {2009}
}
Comments
14 pages, 3 figures, 1 table, accepted to AJ