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The variable “hybrid” PG 1159 star HS 2324+3944
Published online by Cambridge University Press: 25 May 2016
Extract
HS 2324+3944 is one of only four “hybrid” PG 1159 stars. The latter objects are a subgroup of DO white dwarfs. The spectra of “hybrids” show an He ii/C iv absorption trough similar to the “classical” PG 1159 stars, but also strong Balmer lines (Napiwotzki & Schönberner 1991).
- Type
- III. Central Stars
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- Copyright © Kluwer 1997
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