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[vsnet-newvar 484] New variable star MisV0957
- Date: Thu, 6 Jul 2000 23:09:59 -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 484] New variable star MisV0957
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV0957).
MisV0957
R.A. 18h29m09s.32
Decl. +04o51'17".6 (2000.0)
Mag. 12.3C-13.5C
Type SR?
= USNO-A2.0_0900.12959112 18 29 09.321 +04 51 17.63 13.6R 16.9B
= IRAS 18266+0449 R.A.=18 29 08.91 Decl.=+04 51 14.8 (22 x 5", p.a.=84) flux(12)=1.93 flux(25)=0.86 flux(60)=<0.45 flux(100)=<16.28 21% variable
http://vsnet.aerith.net/misao/data/MisV/MisV0957.gif
MisV0957 19990605.65144 130C Mis image="KenIchi Kadota"
MisV0957 19990605.65189 129C Mis image="KenIchi Kadota"
MisV0957 19990831.61456 135C Mis image="KenIchi Kadota"
MisV0957 20000523.59351 123C Mis image="Nobuo Ohkura"
MisV0957 20000523.59536 123C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0957.
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