The Spectral Variability of Pulsating Stars: PG1159-035
| dc.creator | Stahn, T. | |
| dc.creator | Dreizler, S. | |
| dc.creator | Werner, K. | |
| dc.date | 2005-02-01 | |
| dc.date.accessioned | 2026-07-07T02:16:54Z | |
| dc.date.available | 2026-07-07T02:16:54Z | |
| dc.description | 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 516s 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. | |
| dc.description | 4 pages, 3 figures, requires asp2004.sty, to appear in the proceedings of the 14th European Workshop on White Dwarfs, eds. D. Koester and S. Moehler, ASP Conf. Ser | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0502013 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0502013 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/8968 | |
| dc.subject | Astrophysics | |
| dc.title | The Spectral Variability of Pulsating Stars: PG1159-035 | |
| dc.type | text |