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[vsnet-newvar 822] New variable star MisV1064
- Date: Wed, 18 Apr 2001 20:45:53 -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 822] New variable star MisV1064
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1064).
MisV1064
R.A. 21h56m50s.35
Decl. +55o14'22".4 (2000.0)
Mag. 12.5-14.6C
Type SR:
= USNO-A2.0 1425.12555658 21h56m50s.311 +55o14'22".22 Mag(R):16.0 Mag(B):19.5
= IRAS 21551+5500 21h56m50s.4 +55o14'22" Ellipse:8x4" P.A.:4 Flux(12):1.874 Flux(25):0.8170 Flux(60):<0.5751 Flux(100):<24.71 Var:6%
http://vsnet.aerith.net/misao/data/MisV/MisV1064.gif
MisV1064 19990520.77319 12.55C Mis KAF-1600 - KenIchi_Kadota
MisV1064 19990520.77362 12.50C Mis KAF-1600 - KenIchi_Kadota
MisV1064 19990709.69525 13.95C Mis KAF-1600 - KenIchi_Kadota
MisV1064 19990709.69569 13.66C Mis KAF-1600 - KenIchi_Kadota
MisV1064 19990817.76182 13.46C Mis KAF-1600 - KenIchi_Kadota
MisV1064 19990817.76227 13.63C Mis KAF-1600 - KenIchi_Kadota
MisV1064 19990821.73261 14.37C Mis KAF-1600 - KenIchi_Kadota
MisV1064 19990821.73306 14.54C Mis KAF-1600 - KenIchi_Kadota
MisV1064 19990831.65364 14.26C Mis KAF-1600 - KenIchi_Kadota
MisV1064 19990831.65404 14.17C Mis KAF-1600 - KenIchi_Kadota
MisV1064 19990912.74142 14.64C Mis KAF-1600 - KenIchi_Kadota
MisV1064 19990912.74202 13.71C Mis KAF-1600 - KenIchi_Kadota
MisV1064 19990923.51293 13.65C Mis KAF-1600 - KenIchi_Kadota
MisV1064 19990923.51337 13.39C Mis KAF-1600 - KenIchi_Kadota
MisV1064 20000829.50909 13.53C Mis KAF-1600 - Nobuo_Ohkura
MisV1064 20000829.51094 13.43C Mis KAF-1600 - Nobuo_Ohkura
MisV1064 20000829.51279 13.53C Mis KAF-1600 - Nobuo_Ohkura
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1064.
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/
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp