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[vsnet-newvar 627] New variable star MisV1036
- Date: Thu, 12 Oct 2000 22:19:16 -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 627] New variable star MisV1036
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1036).
MisV1036
R.A. 22h07m20s.98
Decl. +40o48'50".6 (2000.0)
Mag. 10.7C-12.4C
Type ?
= USNO-A2.0_1275.17057902 22 07 20.976 +40 48 50.60 15.0R 18.7B
= IRAS 22052+4034 R.A.=22 07 20.07 Decl.=+40 48 42.4 (22 x 7", p.a.=57) flux(12)=11.64 flux(25)=7.37 flux(60)=1.08 flux(100)=2.12 17% variable
http://vsnet.aerith.net/misao/data/MisV/MisV1036.gif
MisV1036 19990312.82990 108C Mis image="KenIchi Kadota"
MisV1036 19990312.83234 108C Mis image="KenIchi Kadota"
MisV1036 19990312.83333 107C Mis image="KenIchi Kadota"
MisV1036 20000807.53134 124C Mis image="Nobuo Ohkura"
MisV1036 20000807.53319 124C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1036.
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/
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp