[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-newvar 521] New variable star MisV0972
- Date: Thu, 10 Aug 2000 21:22:53 -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 521] New variable star MisV0972
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV0972).
MisV0972
R.A. 19h31m11s.37
Decl. +25o17'46".0 (2000.0)
Mag. 13.0C-13.9C
Type SR?
= IRAS 19291+2511 R.A.=19 31 10.63 Decl.=+25 17 41.1 (18 x 4", p.a.=71) flux(12)=5.73 flux(25)=3.16 flux(60)=<0.42 flux(100)=<4.91 18% variable
= 2MASS 193111.343 +251745.07 (2000.0) 8.397 7.141 6.271
http://vsnet.aerith.net/misao/data/MisV/MisV0972.gif
MisV0972 19990605.70681 138C Mis image="KenIchi Kadota"
MisV0972 19990605.70726 139C Mis image="KenIchi Kadota"
MisV0972 20000613.63123 130C Mis image="Nobuo Ohkura"
MisV0972 20000613.63308 130C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0972.
It was picked up by Yoshida from the candidates of new variable stars
detected by the PIXY system from images taken by Ohkura comparing with
images taken by Kadota. Kadota and Yoshida judged it as a real
variable star.
The magnitude are measured automatically by the PIXY system. Image
observers' names are noted after "Mis".
The identification with the 2MASS data is by Taichi Kato.
Please see the URL below for the MISAO Project and the PIXY system.
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