Soft X-ray Spectroscopy of the Hot DA White Dwarf LB1919 and the PG1159 Star PG1520+525

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dc.creatorWerner, K.
dc.creatorDrake, J. J.
dc.creatorRauch, T.
dc.creatorSchuh, S.
dc.creatorGautschy, A.
dc.date2006-09-30
dc.date.accessioned2026-07-07T07:26:49Z
dc.date.available2026-07-07T07:26:49Z
dc.descriptionWe have performed soft X-ray spectroscopy of two hot white dwarfs with the Chandra observatory using the Low Energy Transmission Grating. The first target is the hot DA white dwarf LB1919 (Teff=69000 K). This star is representative of a small group of hot DAs whose metallicities lie well below predictions from radiative levitation theory. The Chandra spectrum shows a rich absorption line spectrum which may allow to find the origin of the low-metallicity nature of these DAs. The second target is PG1520+525, a very hot non-pulsating PG1159 star. We find that it is hotter (Teff=150 000 K) than the pulsating prototype PG1159-035 (Teff=140 000) and conclude that both stars confine the blue edge of the GW Vir instability strip.
dc.description6 pages, Proceedings, 15th European Workshop on White Dwarfs
dc.identifierhttps://arxiv.org/abs/astro-ph/0610013
dc.identifierhttp://arxiv.org/abs/astro-ph/0610013
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/117162
dc.subjectAstrophysics
dc.titleSoft X-ray Spectroscopy of the Hot DA White Dwarf LB1919 and the PG1159 Star PG1520+525
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