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[vsnet-chat 155] Re: V1504 Cyg
- Date: Fri, 28 Feb 1997 22:44:12 +0900 (JST)
- To: vsnet-chat
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-chat 155] Re: V1504 Cyg
- Cc: e.kuulkers1@physics.oxford.ac.uk
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Erik Kuulkers wrote:
> V1504 Cyg has been put forward as a SU UMa star, just because it shows
> long and short outbursts (see Raykov & Yushchenko 1988, Perem. Zvezdy,
> 22, 853).
Yes, the SU UMa-type nature of V1504 Cyg was revealed and already announced
by the Ouda group via VSNET. I've heard Nogam-san is writing a paper on
this -- he may provide more info.
> However, in the VSNET database this star is still classified as "UGZ:".
> Does anyone have more information on this star, or are there extensive
> observations available during long (super?) outbursts, which may point to
> the existence of superhumps?
The variable-type database used to draw VSNET light curves is already
a little too obsolete, but I don't not have yet time to revise it. Actually
it's UGSU.
Regard,
Taichi Kato
Return to Daisaku Nogami
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