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[vsnet-j 2250] Re: Nova candidate
- Date: Mon, 16 Sep 2002 13:13:54 +0900 (JST)
- To: vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp, vsnet-campaign-nova@ooruri.kusastro.kyoto-u.ac.jp, vsnet-discovery-nova@ooruri.kusastro.kyoto-u.ac.jp, vsnet-j@ooruri.kusastro.kyoto-u.ac.jp, vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
- From: Hitoshi YAMAOKA <yamaoka@rc.kyushu-u.ac.jp>
- Subject: [vsnet-j 2250] Re: Nova candidate
- Sender: owner-vsnet-j@ooruri.kusastro.kyoto-u.ac.jp
Re: Nova candidate
>180220.7 -251751 (2000.0) IRAS17592-2517 10.920 6.981 24.840L 440.400L 97%
>180220.7 -251751 (2000.0) SSC17592-2517 10.920 6.981 24.840L 440.400L
>180221.0 -251749 (2000.0) MSX5C_G005.0235-01.3649 -15 -8 7 8 6 6 V(%):-:-:2:5:3:3
Probable optical counterpart of this IR source is very dim even on DSS
2 red plate. It is marginally catalogued as:
USNO_A2.0 18:02:20.746 -25:17:51.79 r=17.6 b=20.1
GSC_2.2 18:02:20.732 -25:17:50.99 r=17.93
If it is a true counterpart of the new object, the brightening in V
well exceed 10 magnitude.
Sincerely Yours,
Hitoshi Yamaoka, Kyushu Univ., Japan
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