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[vsnet-newvar 604] New variable star MisV1013
- Date: Thu, 12 Oct 2000 20:24:42 -0500
- To: dubois@simbad.u-strasbg.fr, gerard@simbad.u-strasbg.fr, samus@sai.msu.ru, vsnet-newvar@kusastro.kyoto-u.ac.jp
- From: Seiichi Yoshida <comet@aerith.net>
- Subject: [vsnet-newvar 604] New variable star MisV1013
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1013).
MisV1013
R.A. 20h09m28s.44
Decl. +30o16'20".6 (2000.0)
Mag. 9.4C-10.5C
Type ?
= USNO-A2.0_1200.14578891 20 09 28.443 +30 16 20.61 12.5R 16.1B
= IRAS 20074+3007 R.A.=20 09 27.89 Decl.=+30 16 17.8 (20 x 5", p.a.=70) flux(12)=3.89 flux(25)=1.79 flux(60)=<3.98 flux(100)=<53.33 29% variable
http://vsnet.aerith.net/misao/data/MisV/MisV1013.gif
MisV1013 19990715.65855 101C Mis blending image="KenIchi Kadota"
MisV1013 19990715.65902 104C Mis image="KenIchi Kadota"
MisV1013 19990803.67126 105C Mis image="KenIchi Kadota"
MisV1013 19990803.67419 105C Mis image="KenIchi Kadota"
MisV1013 20000706.60259 94C Mis image="Nobuo Ohkura"
MisV1013 20000706.60443 98C Mis blending image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1013.
It was picked up by Yoshida from the candidates of new variable stars
detected by the PIXY system from images taken by Ohkura comparing with
images taken by Kadota. Kadota and Yoshida judged it as a real
variable star.
The magnitude are measured automatically by the PIXY system. Image
observers' names are noted after "Mis".
Please see the URL below for the MISAO Project and the PIXY system.
http://vsnet.aerith.net/misao/
--
Seiichi Yoshida
comet@aerith.net
http://vsnet.aerith.net/
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vsnet-adm@kusastro.kyoto-u.ac.jp