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arXiv · 1609.08683

On the formation of DA white dwarfs with low hydrogen contents: Preliminary Results

M. M. Miller Bertolami·L. G. Althaus·A. H. Córsico
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Abstract

Systematic photometric and asteroseismological studies in the last decade support the belief that white dwarfs in the solar neighborhood harbor a broad range of hydrogen-layer contents. The reasons behind this spread of hydrogen-layer masses are not understood and usually misunderstood. In this work we present, and review, the different mechanisms that can (or cannot) lead to the formation of white dwarfs with a broad range hydrogen contents.

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M. M. Miller Bertolami, L. G. Althaus, A. H. Córsico. 2016-09-27. On the formation of DA white dwarfs with low hydrogen contents: Preliminary Results. https://arxiv.org/abs/1609.08683

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