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[vsnet-newvar 793] New variable star MisV1051
- Date: Wed, 21 Mar 2001 22:18:34 -0600
- 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 793] New variable star MisV1051
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1051).
MisV1051
R.A. 20h13m51s.28
Decl. +41o45'35".4 (2000.0)
Mag. 11.8-12.6C
Type ?
= IRAS 20120+4136 20h13m49s.6 +41o45'25" Ellipse:13x5" P.A.:65 Flux(12):6.151 Flux(25):3.515 Flux(60):<15.25 Flux(100):59.12 Var:6%
http://vsnet.aerith.net/misao/data/MisV/MisV1051.gif
MisV1051 19990803.68972 12.64C Mis KAF-1600 - KenIchi_Kadota
MisV1051 19990803.69016 12.62C Mis KAF-1600 - KenIchi_Kadota
MisV1051 19991121.42156 11.88C Mis KAF-1600 - KenIchi_Kadota
MisV1051 19991121.42201 11.83C Mis KAF-1600 - KenIchi_Kadota
Seiichi Yoshida, MISAO Project; and KenIchi Kadota, Ageo, Saitama,
Japan, discovered a new variable star MisV1051.
It was picked up by Seiichih Yoshida from the candidates of new
variable stars detected by the PIXY system 2 from images taken by
KenIchi Kadota, and confirmed by KenIchi Kadota.
The identification is researched by Taichi Kato (Kyoto University),
John Greaves (the United Kingdom), and Seiichi Yoshida.
The magnitude are measured automatically by the PIXY system 2.
About the MISAO Project and the PIXY system 2:
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