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[vsnet-newvar 491] New variable star MisV0964
- Date: Thu, 6 Jul 2000 23:47:59 -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 491] New variable star MisV0964
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV0964).
MisV0964
R.A. 19h20m59s.12
Decl. +04o41'20".3 (2000.0)
Mag. 12.8C-14.8C
Type ?
= USNO-A2.0_0900.14708192 19 20 59.135 +04 41 24.68 16.2R 19.7B
= IRAS 19185+0435 R.A.=19 21 00.62 Decl.=+04 41 27.9 (71 x 12", p.a.=80) flux(12)=0.32 flux(25)=<0.25 flux(60)=<0.44 flux(100)=<15.06
http://vsnet.aerith.net/misao/data/MisV/MisV0964.gif
MisV0964 20000216.82586 144C Mis image="KenIchi Kadota"
MisV0964 20000216.82875 148C Mis image="KenIchi Kadota"
MisV0964 20000216.83083 147C Mis image="KenIchi Kadota"
MisV0964 20000523.62500 129C Mis image="Nobuo Ohkura"
MisV0964 20000523.62686 128C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0964.
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