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[vsnet-chat 2991] Re: R CrB stars
- Date: Sun, 28 May 2000 21:56:34 +0900 (JST)
- To: vsnet-chat
- From: Taichi Kato <tkato>
- Subject: [vsnet-chat 2991] Re: R CrB stars
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Re: R CrB stars
> There are not R Cor Bor type stars.
> There are stars with the R CrB type variablity!
Whether it will be adequate or not to call sudden fadings caused by
dust formation as the R CrB type variablity, this process has been widely
observed in different sort of objects (R CrB stars themselves, carbon stars,
RVB minimum (possible), DQ Her-type novae etc.).
However, the population of R CrB stars definitely exists, sharing some
common characterstics (see Clayton's review). It is not clear whether
this class of variable represents a single or multiple classes of objects
(e.g. in evolution), or whether the class has a definite borderline between
R CrB stars and other variable stars.
Regards,
Taichi Kato
Return to Daisaku Nogami
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