The Spectral variability of pulsating stars: PG1159-035
Feb, 20054 pages
Part of Proceedings, 14th European White Dwarf Workshop (EUROWD 04) : Kiel, Germany, July 19-23, 2004, 545
Published in:
- ASP Conf.Ser. 334 (2005) 545
Contribution to:
- , 545
- EUROWD 04
- Published: 2005
e-Print:
- astro-ph/0502013 [astro-ph]
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Abstract: (Astronomical Society of the Pacific)
With 10m class telescopes as well as with time-tagging detectors on board of HST and FUSE, the analysis of time-resolved spectra for pulsating white dwarfs becomes feasible. We present simulated time-resolved spectra for the hot pulsating white dwarf PG1159−035 and compare these models with observational data of the 516 s mode based on HST-STIS spectroscopy. A determination of the pulsation mode by the spectral variability of PG1159−035 seems to be impossible for the moment.References(5)
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