A comparison of DA white dwarf temperatures and gravities from Lyman and Balmer line studies
Open Access
- 1 November 2001
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 328 (1) , 211-222
- https://doi.org/10.1046/j.1365-8711.2001.04855.x
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This publication has 27 references indexed in Scilit:
- Adding More Mysteries to the DA White Dwarf GD 394The Astrophysical Journal, 2000
- Comparison of White Dwarf Models with STIS SpectrophotometryThe Astronomical Journal, 2000
- Evidence for the stratification of Fe in the photosphere of G191 B2BMonthly Notices of the Royal Astronomical Society, 1999
- The effect of photospheric heavy elements on the hot DA white dwarf temperature scaleMonthly Notices of the Royal Astronomical Society, 1998
- Properties of the Hot DA White Dwarf HZ 43 Based on Far-Ultraviolet [ITAL]ORFEUS[/ITAL]-[ITAL]SPAS II[/ITAL] ObservationsThe Astrophysical Journal, 1998
- The mass, temperature and distance of the white dwarf in V471 TauriMonthly Notices of the Royal Astronomical Society, 1997
- A search for hidden white dwarfs in the ROSAT extreme ultraviolet surveyMonthly Notices of the Royal Astronomical Society, 1997
- RE 1738 + 665: the hottest DA white dwarf detected by ROSATMonthly Notices of the Royal Astronomical Society, 1994
- A new hot DA white dwarf in a region of exeptionally low H I densityMonthly Notices of the Royal Astronomical Society, 1994
- A spectroscopic determination of the mass distribution of DA white dwarfsThe Astrophysical Journal, 1992