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[vsnet-newvar 566] New variable star MisV0992
- Date: Tue, 5 Sep 2000 21:37:12 -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 566] New variable star MisV0992
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV0992).
MisV0992
R.A. 19h44m55s.30
Decl. +17o40'24".3 (2000.0)
Mag. 12.1C-14.1C
Type SR?
= IRAS 19426+1733 R.A.=19 44 55.65 Decl.=+17 40 27.6 (28 x 7", p.a.=72) flux(12)=2.25 flux(25)=1.46 flux(60)=<0.43 flux(100)=<17.44 99% variable
= 2MASS 194455.252 +174024.47 (2000.0) 8.408 7.150 6.271
http://vsnet.aerith.net/misao/data/MisV/MisV0992.gif
MisV0992 19990715.63538 141C Mis image="KenIchi Kadota"
MisV0992 19990715.63604 141C Mis image="KenIchi Kadota"
MisV0992 20000525.67079 123C Mis image="Nobuo Ohkura"
MisV0992 20000525.67264 121C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0992.
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