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[vsnet-newvar 621] New variable star MisV1030
- Date: Thu, 12 Oct 2000 21:49:52 -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 621] New variable star MisV1030
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1030).
MisV1030
R.A. 20h31m21s.00
Decl. +33o36'46".8 (2000.0)
Mag. 12.4C-13.8C
Type ?
= USNO-A2.0_1200.15249451 20 31 20.995 +33 36 46.75 14.5R 17.4B
= IRAS 20293+3326 R.A.=20 31 21.64 Decl.=+33 36 49.4 (23 x 9", p.a.=68) flux(12)=0.97 flux(25)=0.51 flux(60)=<1.60 flux(100)=<79.05 93% variable
http://vsnet.aerith.net/misao/data/MisV/MisV1030.gif
MisV1030 19990605.74081 137C Mis image="KenIchi Kadota"
MisV1030 19990605.74134 138C Mis image="KenIchi Kadota"
MisV1030 20000803.53734 124C Mis image="Nobuo Ohkura"
MisV1030 20000803.53919 125C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1030.
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".
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