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[vsnet-chat 2559] TmzV631
- Date: Sat, 15 Jan 2000 02:18:49 +0200 (EET)
- To: vsnet-chat@kusastro.kyoto-u.ac.jp
- From: stars@personal.eunet.fi (Timo Kinnunen)
- Subject: [vsnet-chat 2559] TmzV631
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
> Kesao Takamizawa (Nagano, Japan) reports the discovery of a new variable
>star (TmzV631). The IRAS color looks peculiar for a normal star. The USNO
>color is not very markedly red. Has anyone suggestions on the classification?
While polishing my data on Sonneberg variables, just a few days ago
I stumbled on also somewhat peculiar BS Cep. On SIMBAD it is a dwarf
nova. At first sight the DSS image looked similar to BZ Cam.
But BS Cep has also a remarkable coincident IRAS source.
BS Cep is discussed in:
> 1992A&AS...93..419B
>Spectroscopy of poorly known northern dwarf novae. Part II.
> BRUCH A., SCHIMPKE T.
and reclassified as a Herbig emission star (HES).
This class is still obscure to me. Other representatives?
Well, perhaps TmzV631 and BS Cep are related!
Regards,
Timo Kinnunen
Return to Daisaku Nogami
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