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[vsnet-campaign-dn 3518] V2276 Sgr and YY Tel
- Date: Tue, 4 Mar 2003 12:07:44 +0900 (JST)
- To: vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp,vsnet-gcvs@ooruri.kusastro.kyoto-u.ac.jp,vsnet-id@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-campaign-dn 3518] V2276 Sgr and YY Tel
- Delivered-To: vsnet-campaign-dn-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp
V2276 Sgr and YY Tel
According to astro-ph/0303022 (Mason and Howell), V2276 Sgr was given
a spectroscopic classification of a DC white dwarf. From the VSNET
record, the object unmistakably underwent outbursts. The case looks
similar to CG CMa, for which a misidentified nearby star was given a
spectroscopic classification of a white dwarf (see Kato et al. 1999, IBVS
No. 4760 and Duerbeck et al. 1999 IBVS No. 4759). V2276 Sgr warrants
further study, and a new exact identification using outburst images.
The same is true for YY Tel, which is reported to lack emission lines.
Regards,
Taichi Kato
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