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Talk:Pulsating white dwarf

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This is the current revision of this page, as edited by Cewbot (talk | contribs) at 13:27, 8 February 2024 (Maintain {{WPBS}} and vital articles: 1 WikiProject template. Create {{WPBS}}. Keep majority rating "Start" in {{WPBS}}. Remove 1 same rating as {{WPBS}} in {{WPAstronomy}}.). The present address (URL) is a permanent link to this version.
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Comments

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Comment. I have followed Quirion et al., ApJS 171, 219 and Nagel and Werner, A&A 426, L45 in including some non-PG 1159 stars in the class of GW Vir stars. Spacepotato 02:47, 20 September 2007 (UTC) The article has been rewritten. Spacepotato 16:25, 20 September 2007 (UTC)[reply]

GW Vir variables - relocate to "PG 1159 star"?

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As almost all GW Vir variables are PG 1159 stars, rather than bona fide white dwarfs, wouldn't it make more sense to cover them in the PG 1159 star article instead? It seems like it would make sense to discuss only the rare GW Vir white dwarfs here, with a link to coverage of non-WD GW Vir stars on the PG 1159 page. --203.57.213.46 (talk) 06:05, 24 November 2014 (UTC)[reply]