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Broadening of Ly α by neutral helium in DBA white dwarfs

Gänsicke, BT; Koester, D; Farihi, J; Toloza, O; (2018) Broadening of Ly α by neutral helium in DBA white dwarfs. Monthly Notices of the Royal Astronomical Society , 481 (4) pp. 4323-4331. 10.1093/mnras/sty2526. Green open access

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Abstract

Traces of photospheric hydrogen are detected in at least half of all white dwarfs with heliumdominated atmospheres through the presence of Hα in high-quality optical spectroscopy. Previous studies have noted significant discrepancies between the hydrogen abundances derived from Hα and Ly α for a number of stars where ultraviolet spectroscopy is also available. We demonstrate that this discrepancy is caused by inadequate treatment of the broadening of Ly α by neutral helium. When fitting Hubble Space Telescope far-ultraviolet spectroscopy of 17 DB white dwarfs using our new line profile calculations, we find good agreement between log (NH/NHe) measured from Ly α and Hα. Larger values of log (NH/NHe) based on Ly α are still found for three stars, which are among the most distant in our sample, and we show that a small amount of interstellar absorption from neutral hydrogen can account for this discrepancy.

Type: Article
Title: Broadening of Ly α by neutral helium in DBA white dwarfs
Open access status: An open access version is available from UCL Discovery
DOI: 10.1093/mnras/sty2526
Publisher version: http://dx.doi.org/10.1093/mnras/sty2526
Language: English
Additional information: © 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: line: profiles, stars: atmospheres, white dwarfs, ultraviolet: stars
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery.ucl.ac.uk/id/eprint/10059679
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