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[vsnet-newvar 788] New variable star MisV1046
- Date: Sun, 18 Mar 2001 19:35:40 -0600
- 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 788] New variable star MisV1046
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1046).
MisV1046
R.A. 19h59m49s.83
Decl. +43o28'37".4 (2000.0)
Mag. 12.6-13.0C
Type SR?
= USNO-A2.0 1275.13021417 19h59m49s.613 +43o28'37".87 Mag(R):15.1 Mag(B):18.2
= 2MASS 195949.673 +432837.38 (2000.0) 8.379 7.278 6.819
http://vsnet.aerith.net/misao/data/MisV/MisV1046.gif
MisV1046 19990724.58585 12.92C Mis KAF-1600 - KenIchi_Kadota
MisV1046 19990724.58665 13.03C Mis KAF-1600 - KenIchi_Kadota
MisV1046 20000904.46388 12.56C Mis KAF-1600 - Nobuo_Ohkura
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1046.
It was picked up by Seiichih 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