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[vsnet-newvar 487] New variable star MisV0960
- Date: Thu, 6 Jul 2000 23:27:58 -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 487] New variable star MisV0960
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV0960).
MisV0960
R.A. 18h30m28s.43
Decl. +05o23'32".4 (2000.0)
Mag. 12.7C-13.9C
Type ?
= GSC0454.1651 18 30 28.40 +05 23 31.4 13.87
= USNO-A2.0_0900.13020656 18 30 28.431 +05 23 32.37 12.8R 14.7B
= IRAS 18280+0521 R.A.=18 30 28.09 Decl.=+05 23 35.5 (30 x 7", p.a.=85) flux(12)=12.14 flux(25)=7.95 flux(60)=1.96 flux(100)=<2.56 93% variable
http://vsnet.aerith.net/misao/data/MisV/MisV0960.gif
MisV0960 19990605.65144 129C Mis image="KenIchi Kadota"
MisV0960 19990605.65189 129C Mis image="KenIchi Kadota"
MisV0960 19990831.61456 127C Mis image="KenIchi Kadota"
MisV0960 20000523.59351 137C Mis image="Nobuo Ohkura"
MisV0960 20000523.59536 139C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0960.
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