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[vsnet-newvar 516] New variable star MisV0967
- Date: Thu, 10 Aug 2000 20:57:54 -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 516] New variable star MisV0967
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV0967).
MisV0967
R.A. 21h01m29s.92
Decl. +25o03'43".1 (2000.0)
Mag. 9.9C-10.7C
Type SR?
= GSC2176.1341 21 01 29.95 +25 03 42.6 12.06
= USNO-A2.0_1125.17665378 21 01 29.921 +25 03 43.05 11.2R 14.3B
= IRAS 20593+2451 R.A.=21 01 30.57 Decl.=+25 03 45.0 (41 x 6", p.a.=68) flux(12)=1.55 flux(25)=0.69 flux(60)=<0.40 flux(100)=<1.00 1% variable
= 2MASS 210129.896 +250342.81 (2000.0) 6.360 5.460 4.956
= 2MASS 210129.952 +250342.48 (2000.0) 0.000 0.000 0.000
http://vsnet.aerith.net/misao/data/MisV/MisV0967.gif
MisV0967 19990724.61215 107C Mis image="KenIchi Kadota"
MisV0967 19990724.61257 106C Mis image="KenIchi Kadota"
MisV0967 20000613.68705 99C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0967.
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