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[vsnet-alert 7014] Re: Possible nova in Mon
- Date: Sat, 12 Jan 2002 18:08:14 +0900 (JST)
- To: vsnet-alert@kusastro.kyoto-u.ac.jp, vsnet-campaign-nova@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-alert 7014] Re: Possible nova in Mon
- Sender: owner-vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
Re: Possible nova in Mon
Arne Henden wrote:
> The actual photometry of the possible nova itself is:
> RA (J2000) DEC HJD V B-V U-B V-R R-I
> 106.020068 -3.847484 52285.7223 9.975 1.726 1.916 0.943 0.931
> with internal astrometric errors of about 100mas and external
> photometric errors of about 0.03mag due to the poor seeing.
> ((U-B) is more suspect than the other colors because of the
> crowded field.) This does not look nova-like to me.
The color seems to be on a smooth extension of late-type Barium stars.
The expanded photosphere may somehow mimic a late-type Barium star both in
spectrum and colors.
Regards,
Taichi Kato
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