WD1032+011, an inflated brown dwarf in an old eclipsing binary with a white dwarf
arXiv:2006.09417 · doi:10.1093/mnras/staa1608
Abstract
We present the discovery of only the third brown dwarf known to eclipse a non-accreting white dwarf. Gaia parallax information and multi-colour photometry confirm that the white dwarf is cool (9950150K) and has a low mass (0.450.05~MSun), and spectra and lightcurves suggest the brown dwarf has a mass of 0.067 0.006 MSun (70 MJup) and a spectral type of L5 1. The kinematics of the system show that the binary is likely to be a member of the thick disk and therefore at least 5 Gyr old. The high cadence lightcurves show that the brown dwarf is inflated, making it the first brown dwarf in an eclipsing white dwarf-brown dwarf binary to be so.
arXiv commentAccepted for publication in MNRAS, 11 pages, 7 Figures
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