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[vsnet-newvar 885] New variable star MisV1090
- Date: Tue, 29 May 2001 22:33:06 -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 885] New variable star MisV1090
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1090).
MisV1090
R.A. 19h51m51s.23
Decl. +35o55'57".4 (2000.0)
Mag. 13.0-13.5C
Type ?
= USNO-A2.0 1200.13535959 19h51m51s.191 +35o55'57".31 Mag(R):14.7 Mag(B):17.2
= 2MASS 195151.206 +355557.19 (2000.0) 9.599 8.578 8.154
http://vsnet.aerith.net/misao/data/MisV/MisV1090.gif
MisV1090 19990803.64247 13.52C Mis KAF-1600 - KenIchi_Kadota
MisV1090 19990803.64291 13.48C Mis KAF-1600 - KenIchi_Kadota
MisV1090 20000920.43264 12.97C Mis KAF-1600 - Nobuo_Ohkura
MisV1090 20000920.43451 13.07C Mis KAF-1600 - Nobuo_Ohkura
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1090.
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