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[vsnet-newvar 617] New variable star MisV1026
- Date: Thu, 12 Oct 2000 21:30:24 -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 617] New variable star MisV1026
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1026).
MisV1026
R.A. 20h14m07s.15
Decl. +37o07'13".2 (2000.0)
Mag. 12.4C-14.4C
Type ?
= IRAS 20122+3657 R.A.=20 14 06.77 Decl.=+37 07 09.2 (26 x 3", p.a.=65) flux(12)=1.62 flux(25)=0.88 flux(60)=<6.44 flux(100)=<56.43 98% variable
http://vsnet.aerith.net/misao/data/MisV/MisV1026.gif
MisV1026 19991121.41485 142C Mis image="KenIchi Kadota"
MisV1026 19991121.41586 144C Mis image="KenIchi Kadota"
MisV1026 20000804.52413 124C Mis image="Nobuo Ohkura"
MisV1026 20000804.52598 125C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1026.
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