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[vsnet-chat 979] Re: On the nature of V2323 Sgr
- Date: Tue, 09 Jun 1998 15:36:41 +0900
- To: vsnet-chat@kusastro.kyoto-u.ac.jp
- From: Seiichiro Kiyota <skiyota@abr.affrc.go.jp>
- Subject: [vsnet-chat 979] Re: On the nature of V2323 Sgr
- In-Reply-To: <9806082021.AA14155@runner.nofs.navy.mil>
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
After long bad weather, I could observe V2323 Sgr by CCD in Johnson V and Cousins Rc band as
following.
-------------------------------------------------------
SGRV2323 98 May 21 18h35mUT 11.72C
SGRV2323 98 Jun 07 17h40mUT 12.15Rc
SGRV2323 98 Jun 07 17h50mUT 13.14V
-------------------------------------------------------
C means CCD without filter
Comparison star is GSC6851:2930(V=8.75 B-V=0.005 in Tycho catalog)
V-Rc=0.99 indicates that this star has red color. Usually UG in outburst has not such red
color, so I think that V2323 Sgr is not UG.
V2323 Sgr is discovered by Oosterhoff et al. (1967, Bull. astr. Inst. Nethl. suppl. ser. 67) .
T. Lloyd Evans (1976, MNRAS 174) reported as following;
V2323 Sgr blue star
star indicated by Oosterhoff et al. is not variable on our I plate.
(I don't know exactly but) Evans's article may be reference of classification of V2323 Sgr as
UG: in GCVS. I don't know why the star observed by Evans is blue.
But V2323 Sgr is not blue star in my observation (same as reported by T. Kato, Vsnet-chat
971).
I use the finding chart in catalog of cataclysmic variables (Downs and Shara) for
identification.
Spectroscopy may need to resolve nature of V2323 Sgr.
Seiichiro Kiyota
----
Seiichiro Kiyota skiyota@abr.affrc.go.jp
Laboratory of Stress Physiology
Department of Plant Physiology
National Insititute of Agrobiological Resources
Tel:81-298-38-8384
Fax:81-298-38-8347
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