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[vsnet-newvar 1819] Re: (fwd) ASAS variables: identifications by Anton Paschke
- Date: Sat, 1 Feb 2003 10:17:30 +0900 (JST)
- To: vsnet-gcvs@ooruri.kusastro.kyoto-u.ac.jp,vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp,vsnet-survey@ooruri.kusastro.kyoto-u.ac.jp
- From: Hitoshi YAMAOKA <yamaoka@rc.kyushu-u.ac.jp>
- Subject: [vsnet-newvar 1819] Re: (fwd) ASAS variables: identifications by Anton Paschke
- Cc: Anton_Paschke@swissre.com
- Delivered-To: vsnet-newvar-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
Re: (fwd) ASAS variables: identifications by Anton Paschke
>and is only a few arcminutes from the position of NSV00712. But it
>has an magnitude of 11.3 and NSV00712 is a bright star, magnitude 2.5
NSV 00712 = BD -18 0356 = SAO 148178 is a very red star. Its
magnitude is indeed 2.89-3.02, but in K (infrared) band. Its V and B
magnitudes are 7.05 and 8.66, respectingly.
>so of course they can not be identical.
The conclusion does not change, though.
Sincerely,
Hitoshi Yamaoka
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