Evidence for a merger of binary white dwarfs: the case of GD 362

Details Evidence for a merger of binary white dwarfs: the case of GD 362 Evidence for a merger of binary white dwarfs: the case of GD 362

2007-04-10

arxiv.org/abs/0704.1258v1

Astronomy and Astrophysics

Astrophysics

4 pages, 3 figures. Accepted for publication in Astrophysical Journal Letters

Scientific paper

10.1086/518768

GD 362 is a massive white dwarf with a spectrum suggesting a H-rich atmosphere which also shows very high abundances of Ca, Mg, Fe and other metals. However, for pure H-atmospheres the diffusion timescales are so short that very extreme assumptions have to be made to account for the observed abundances of metals. The most favored hypothesis is that the metals are accreted from either a dusty disk or from an asteroid belt. Here we propose that the envelope of GD 362 is dominated by He, which at these effective temperatures is almost completely invisible in the spectrum. This assumption strongly alleviates the problem, since the diffusion timescales are much larger for He-dominated atmospheres. We also propose that the He-dominated atmosphere of GD 362 is likely to be the result of the merger of a binary white dwarf.

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