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[vsnet-newvar 607] New variable star MisV1016
- Date: Thu, 12 Oct 2000 20:39:18 -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 607] New variable star MisV1016
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1016).
MisV1016
R.A. 20h44m01s.03
Decl. +38o34'23".1 (2000.0)
Mag. 11.9C-14.2C
Type M?
= IRAS 20421+3823 R.A.=20 44 01.60 Decl.=+38 34 22.5 (20 x 7", p.a.=57) flux(12)=1.34 flux(25)=0.82 flux(60)=<7.50 flux(100)=24.47 97% variable
= 2MASS 204400.993 +383423.93 (2000.0) 7.089 5.961 5.304
http://vsnet.aerith.net/misao/data/MisV/MisV1016.gif
MisV1016 19991121.47200 141C Mis image="KenIchi Kadota"
MisV1016 19991121.47242 142C Mis image="KenIchi Kadota"
MisV1016 20000726.55855 120C Mis image="Nobuo Ohkura"
MisV1016 20000726.56041 119C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1016.
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