pith. machine review for the scientific record. sign in

arxiv: astro-ph/0502013 · v1 · submitted 2005-02-01 · 🌌 astro-ph

The Spectral Variability of Pulsating Stars: PG1159-035

T. Stahn (1) , S. Dreizler (1) , K. Werner (2) ((1) Institut fuer Astrophysik , Goettingen , Germany , (2) Institut fuer Astronomie und Astrophysik , Tuebingen , Germany) This is my paper
classification 🌌 astro-ph
keywords pg1159-035pulsatingmodespectraspectraltime-resolvedvariabilitywhite
0
0 comments X
read the original abstract

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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.