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[vsnet-id 743] Re: NSV 4082
- Date: Mon, 3 Feb 2003 19:03:50 +0900 (JST)
- To: gcvs@sai.msu.ru, vsnet-id@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-id 743] Re: NSV 4082
- Delivered-To: vsnet-id-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-id@ooruri.kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-id@ooruri.kusastro.kyoto-u.ac.jp
Re: [vsnet-id 742] NSV 4082
I agree. The ROSAT source is unlikely related.
GSC4853.1862 082626.76 -031743.0 (2000.0) 14.89 0
USNO0825.06329555 082626.714 -031743.27 (2000.0) 14.6 17.6
2MASS 082626.808 -031743.73 (2000.0) 7.166 6.319 5.838
IRAS08239-0307 082355.3 -030747 (1950.0)
F12=0.69 F25=0.25L F60=0.40L F100=1.00L
VAR=-1 LRS=-1
possibly I: oxygen-rich non-variable star without circumstellar shell
or II: variable star with 'young' O-rich circumstellar shell
or VII: variable star with more evolved C-rich circumstellar shell
or VIa: non-variable star with relatively cold dust at large
distance, may be carbon-rich
082625.9 -031740 (2000.0) IRAS08239-0307 0.687 0.250L 0.400L 1.000L -1%
082625.9 -031740 (2000.0) SSC08239-0307 0.687 0.250L 0.400L 1.000L
082626.3 -031743 (2000.0) FSC08239-0307 0.669 0.167 0.175L 0.843L
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