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[vsnet-newvar 612] New variable star MisV1021
- Date: Thu, 12 Oct 2000 21:03:49 -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 612] New variable star MisV1021
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1021).
MisV1021
R.A. 20h10m19s.03
Decl. +30o10'30".4 (2000.0)
Mag. 13.0C-14.9C
Type SR:
= USNO-A2.0_1200.14608798 20 10 19.213 +30 10 30.46 15.0R 17.7B
= 2MASS 201018.956 +301030.52 (2000.0) 8.118 6.598 5.792
http://vsnet.aerith.net/misao/data/MisV/MisV1021.gif
MisV1021 19990611.69750 136C Mis image="KenIchi Kadota"
MisV1021 19990611.70206 135C Mis image="KenIchi Kadota"
MisV1021 19990715.65855 146C Mis image="KenIchi Kadota"
MisV1021 19990715.65902 145C Mis image="KenIchi Kadota"
MisV1021 19990803.67126 149C Mis image="KenIchi Kadota"
MisV1021 20000706.60443 130C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1021.
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