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[vsnet-newvar 606] New variable star MisV1015
- Date: Thu, 12 Oct 2000 20:34:29 -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 606] New variable star MisV1015
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1015).
MisV1015
R.A. 20h43m06s.68
Decl. +30o00'38".8 (2000.0)
Mag. 10.9C-12.3C
Type SR?
= USNO-A2.0_1200.15729247 20 43 06.680 +30 00 38.77 14.3R 18.6B
= IRAS 20410+2949 R.A.=20 43 06.49 Decl.=+30 00 37.2 (28 x 5", p.a.=67) flux(12)=2.26 flux(25)=1.81 flux(60)=<0.42 flux(100)=<11.56 53% variable
= 2MASS 204306.643 +300038.35 (2000.0) 7.428 6.282 5.613
http://vsnet.aerith.net/misao/data/MisV/MisV1015.gif
MisV1015 19991121.48110 109C Mis image="KenIchi Kadota"
MisV1015 19991121.48153 109C Mis image="KenIchi Kadota"
MisV1015 20000706.62297 119C Mis image="Nobuo Ohkura"
MisV1015 20000706.62483 123C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1015.
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 and John
Greaves.
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