T. Rauch(1), K. Werner(1)
(1)Institut für Astronomie und Astrophysik, Astronomie, Universität Tübingen, Waldhäuser Str. 64, D-72076 Tübingen, Germany
Contribution to the 3rd Conference on Faint Blue Stars, Schenectady USA, October 13-17, 1996
Abstract. One of the most interesting spectral classes of immediate white-dwarf progenitors is that of the exotic He-rich PG 1159 stars. We present an analysis of the two brightest PG 1159 stars, the central star of the planetary nebula NGC 246 and of RX J2117.1+3412, and summarize our present picture of post-AGB evolution of He-rich stars.
Paper (245k gzip'ed Postscript including figures)
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Jürgen Barnstedt (barnstedt AT astro.uni-tuebingen.de)
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