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[vsnet-newvar 823] New variable star MisV1066
- Date: Wed, 18 Apr 2001 20:55:52 -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 823] New variable star MisV1066
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1066).
MisV1066
R.A. 22h29m25s.48
Decl. +55o14'04".9 (2000.0)
Mag. 11.3-11.8C
Type ?
= USNO-A2.0 1425.13511025 22h29m25s.471 +55o14'03".95 Mag(R):14.1 Mag(B):17.5
= IRAS 22274+5458 22h29m25s.7 +55o14'05" Ellipse:14x8" P.A.:22 Flux(12):0.5899 Flux(25):0.3095 Flux(60):<1.731 Flux(100):<17.09 Var:0%
http://vsnet.aerith.net/misao/data/MisV/MisV1066.gif
MisV1066 19990709.70923 11.25C Mis KAF-1600 - KenIchi_Kadota
MisV1066 19990709.70966 11.26C Mis KAF-1600 - KenIchi_Kadota
MisV1066 20000829.52950 11.76C Mis KAF-1600 - Nobuo_Ohkura
MisV1066 20000829.53135 11.71C Mis KAF-1600 - Nobuo_Ohkura
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1066.
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