Felix Friederich (1), Thomas Rauch (1), Klaus Werner (1), Lars Koesterke (2) and Jeffrey W. Kruk (3)
1) Institute for Astronomy und Astrophysics, Kepler Center for Astro and Particle Physics,
Eberhard Karls University, D - 72076 Tübingen, Germany
2) Texas Advanced Computer Center, University of Texas, Austin, TX 78758, USA
3) NASA, Goddard Space Flight Center, Greenbelt, MD 20771, USA
To be published in: Proceedings of the 17th European White Dwarf Workshop, AIP Conference Series
Abstract. The central star of the planetary nebula Abell 43 (WD 1751+106) is one of only four known so-called hybrid PG1159 stars. These are hydrogen-deficient due to a late thermal pulse.We present results of a spectral analysis of FUSE, HST /GHRS, and IUE UV observations by means of NLTE model-atmosphere techniques.
Preprint (132 kb PDF file including figures)
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