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[vsnet-newvar 446] New variable star MisV0928
- Date: Wed, 14 Jun 2000 21:26:57 -0500
- To: dubois@simbad.u-strasbg.fr, gerard@simbad.u-strasbg.fr, samus@sai.msu.su, vsnet-newvar@kusastro.kyoto-u.ac.jp
- From: Seiichi Yoshida <comet@aerith.net>
- Subject: [vsnet-newvar 446] New variable star MisV0928
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV0928).
MisV0928
R.A. 19h39m15s.28
Decl. +15o44'34".4 (2000.0)
Mag. 11.0C-14.6C
Type ?
= USNO-A2.0_1050.14326084 19 39 15.277 +15 44 34.36 14.5R 18.0B
= IRAS 19369+1537 R.A.=19 39 14.26 Decl.=+15 44 29.0 (37 x 6", p.a.=74) flux(12)=2.12 flux(25)=1.03 flux(60)=<0.40 flux(100)=<7.74 15% variable
http://vsnet.aerith.net/misao/data/MisV/MisV0928.gif
MisV0928 19990715.61840 110C Mis image="KenIchi Kadota"
MisV0928 19990715.63223 111C Mis image="KenIchi Kadota"
MisV0928 19990715.63291 111C Mis image="KenIchi Kadota"
MisV0928 20000509.63135 146C Mis image="Nobuo Ohkura"
MisV0928 20000509.63321 144C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0928.
It was detected by the PIXY system as one of the candidates of new
variable stars from images taken by Ohkura comparing with images taken
by Kadota, then confirmed by Yoshida.
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