The mass of the white dwarf in GW Libra
Solar and Stellar Astrophysics
2015-05-18 v1
Abstract
We report a mass and rotational broadening (vsini) for the pulsating white dwarf component of the WZ Sge type Dwarf Nova GW Lib based on high-resolution VLT spectroscopy that resolves the MgII 4481A absorption feature. Its gravitational redshift combined with white dwarf mass-radius models, provides us with a direct measurement of the white dwarf mass of M_1 = 0.84 pm 0.02 M_sun. The line is clearly resolved and if associated with rotational broadening gives vsini=87.0 pm 3.4 km/s, equivalent to a spin period of 97 pm 12s.
Keywords
Cite
@article{arxiv.1004.3065,
title = {The mass of the white dwarf in GW Libra},
author = {L. van Spaandonk and D. Steeghs and T. R. Marsh and S. G. Parsons},
journal= {arXiv preprint arXiv:1004.3065},
year = {2015}
}
Comments
16 pages, 2 figures, 2 tables, ApJ letter accepted