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arxiv: 1302.6619 · v1 · pith:6UTFKB3G · submitted 2013-02-26 · astro-ph.SR

Discovery of Molecular Hydrogen in White Dwarf Atmospheres

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classification astro-ph.SR
keywords whiteatmospheresdiscoverydwarfshydrogenmolecularbelowconstraints
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With the Cosmic Origins Spectrograph onboard the Hubble Space Telescope, we have detected molecular hydrogen in the atmospheres of three white dwarfs with effective temperatures below 14,000 K, G29-38, GD 133 and GD 31. This discovery provides new independent constraints on the stellar temperature and surface gravity of white dwarfs.

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Cited by 1 Pith paper

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  1. White dwarfs within 13 pc: Insights from ultraviolet spectroscopy

    astro-ph.SR 2026-07 conditional novelty 6.0

    UV spectroscopy of the 44 nearest white dwarfs reveals a 2–6% temperature discrepancy between UV and optical model fits, six UV-only metal detections, and a 30% planetary debris accretion rate.