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[vsnet-newvar 574] New variable star MisV1000
- Date: Tue, 5 Sep 2000 22:17:13 -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 574] New variable star MisV1000
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1000).
MisV1000
R.A. 20h12m51s.13
Decl. +26o42'04".1 (2000.0)
Mag. 12.1C-13.2C
Type ?
= USNO-A2.0_1125.15334491 20 12 51.119 +26 42 06.27 15.4R 19.0B
= IRAS 20107+2632 R.A.=20 12 50.82 Decl.=+26 42 03.1 (16 x 8", p.a.=67) flux(12)=0.49 flux(25)=0.31 flux(60)=<0.44 flux(100)=<3.76 79% variable
http://vsnet.aerith.net/misao/data/MisV/MisV1000.gif
MisV1000 19990715.65545 132C Mis image="KenIchi Kadota"
MisV1000 19990715.65588 131C Mis image="KenIchi Kadota"
MisV1000 19991121.40282 126C Mis image="KenIchi Kadota"
MisV1000 19991121.40326 127C Mis image="KenIchi Kadota"
MisV1000 20000615.58345 124C Mis image="Nobuo Ohkura"
MisV1000 20000615.58530 121C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1000.
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