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[vsnet-chat 2985] Re: EsB365 observations and request
- Date: Sun, 28 May 2000 17:52:06 +0900 (JST)
- To: vsnet-chat
- From: Taichi Kato <tkato>
- Subject: [vsnet-chat 2985] Re: EsB365 observations and request
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Re: EsB365 observations and request
Berto Monard wrote:
> For instance V1860 Sgr is also considered a possible RCB and V803 Cen has
> been as well not so long ago.
V1860 Sgr is not presently considered as an R CrB star based on
spectroscopy (see a list in Clayton 1996, PASP 108, 225). The key
discriminating factor is the hydrogen deficiency.
Yet another historically confusing group was the VY Scl-type CV. The
prototype VY Scl was originally discovered as a "blue, high galactic
lattitude" R CrB star. The author of the discovery paper keenly suggested
that there should be two polulations of R CrB stars.
Regards,
Taichi Kato
Return to Daisaku Nogami
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