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[vsnet-newvar 1075] New variable star MisV1146
- Date: Sat, 15 Sep 2001 22:53:38 -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 1075] New variable star MisV1146
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1146).
MisV1146
R.A. 21h55m34s.33
Decl. +50o32'33".6 (2000.0)
Mag. 11.9-12.5C
Type SR:
= USNO-A2.0 1350.15320270 21h55m34s.427 +50o32'34".31 Mag(R):14.0 Mag(B):16.6
= IRAS 21537+5018 21h55m35s.2 +50o32'46" Ellipse:21x8" P.A.:14 Flux(12):0.3155 Flux(25):<0.2839 Flux(60):<0.4000 Flux(100):<7.802
= MSX5C_G096.7093-03.1531 -17 -9 0 0 0 -2 V(%):-:-:3:-:-:-
http://vsnet.aerith.net/misao/data/MisV/MisV1146.gif
MisV1146 19990520.76837 12.33C Mis KAF-1600 - KenIchi_Kadota
MisV1146 19990520.76880 12.27C Mis KAF-1600 - KenIchi_Kadota
MisV1146 19990817.75735 12.20C Mis KAF-1600 - KenIchi_Kadota
MisV1146 19990817.75782 12.25C Mis KAF-1600 - KenIchi_Kadota
MisV1146 19990831.65742 12.39C Mis KAF-1600 - KenIchi_Kadota
MisV1146 19990831.65785 12.44C Mis KAF-1600 - KenIchi_Kadota
MisV1146 19990923.51849 12.48C Mis KAF-1600 - KenIchi_Kadota
MisV1146 19990923.51893 12.46C Mis KAF-1600 - KenIchi_Kadota
MisV1146 20000807.52196 12.10C Mis KAF-1600 - Nobuo_Ohkura
MisV1146 20000807.52381 12.05C Mis KAF-1600 - Nobuo_Ohkura
MisV1146 20000807.52566 12.08C Mis KAF-1600 - Nobuo_Ohkura
MisV1146 20000902.52929 11.89C Mis KAF-1600 - Nobuo_Ohkura
MisV1146 20000902.53114 11.89C Mis KAF-1600 - Nobuo_Ohkura
MisV1146 20000902.53299 11.98C Mis KAF-1600 - Nobuo_Ohkura
MisV1146 20001014.47319 12.07C Mis KAF-1600 - Nobuo_Ohkura
MisV1146 20001014.47505 12.09C Mis KAF-1600 - Nobuo_Ohkura
MisV1146 20001014.47690 12.06C Mis KAF-1600 - Nobuo_Ohkura
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1146.
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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