[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-newvar 444] New variable star MisV0926
- Date: Wed, 14 Jun 2000 21:16:56 -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 444] New variable star MisV0926
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV0926).
MisV0926
R.A. 19h38m57s.37
Decl. +15o01'38".1 (2000.0)
Mag. 13.1C-16.0C
Type ?
= USNO-A2.0_1050.14310169 19 38 57.367 +15 01 38.12 16.2R 18.1B
= IRAS 19366+1454 R.A.=19 38 57.16 Decl.=+15 01 37.9 (23 x 6", p.a.=76) flux(12)=2.15 flux(25)=1.30 flux(60)=<0.44 flux(100)=<19.70 92% variable
http://vsnet.aerith.net/misao/data/MisV/MisV0926.gif
MisV0926 19990715.61795 158C Mis image="KenIchi Kadota"
MisV0926 19990715.61840 160C Mis image="KenIchi Kadota"
MisV0926 20000508.70947 133C Mis image="Nobuo Ohkura"
MisV0926 20000508.71132 131C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0926.
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