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[vsnet-newvar 884] New variable star MisV1089
- Date: Tue, 29 May 2001 22:28:07 -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 884] New variable star MisV1089
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1089).
MisV1089
R.A. 19h58m12s.42
Decl. +35o50'34".8 (2000.0)
Mag. 12.4-12.9C
Type ?
= GSC 2682-00238 19h58m12s.31 +35o50'34".7 Error:0.2" Mag:12.94 MagError:0.41 Band:1 Class:3 Plate:004C Flag:F Epoch:12 AUG 1983
= USNO-A2.0 1200.13994465 19h58m12s.299 +35o50'34".71 Mag(R):12.3 Mag(B):13.7
= 2MASS 195812.780 +355032.51 (2000.0) 9.281 8.117 7.532
http://vsnet.aerith.net/misao/data/MisV/MisV1089.gif
MisV1089 19990430.69374 12.42C Mis KAF-1600 - KenIchi_Kadota
MisV1089 19990430.69417 12.39C Mis KAF-1600 - KenIchi_Kadota
MisV1089 19990707.67965 12.89C Mis KAF-1600 - KenIchi_Kadota
MisV1089 19990707.68009 12.84C Mis KAF-1600 - KenIchi_Kadota
MisV1089 19990801.61065 12.92C Mis KAF-1600 - KenIchi_Kadota
MisV1089 19990801.61109 12.86C Mis KAF-1600 - KenIchi_Kadota
MisV1089 19990803.65726 12.92C Mis KAF-1600 - KenIchi_Kadota
MisV1089 19990803.65770 12.87C Mis KAF-1600 - KenIchi_Kadota
MisV1089 19990831.63196 12.81C Mis KAF-1600 - KenIchi_Kadota
MisV1089 19990831.63242 12.78C Mis KAF-1600 - KenIchi_Kadota
MisV1089 20000920.43636 12.42C Mis KAF-1600 - Nobuo_Ohkura
MisV1089 20000920.43821 12.36C Mis KAF-1600 - Nobuo_Ohkura
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1089.
It was picked up by Seiichi Yoshida from the candidates of new
variable stars detected by the PIXY system 2 from images taken by
Nobuo Ohkura comparing with 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/
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