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[vsnet-newvar 1353] New variable star MisV1149
- Date: Sat, 22 Dec 2001 08:41:28 -0600
- 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 1353] New variable star MisV1149
- Delivered-To: vsnet-newvar@kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV1149).
MisV1149
R.A. 00h22m31s.40
Decl. +56o07'48".3 (2000.0)
Mag. 10.7-11.9C
Type ?
= USNO-A2.0 1425.00526022 00h22m31s.589 +56o07'48".90 Mag(R):11.9 Mag(B):14.6
= IRAS 00198+5551 00h22m31s.3 +56o07'40" Ellipse:20x9" P.A.:34 Flux(12):0.5486 Flux(25):0.3121 Flux(60):<0.4000 Flux(100):<7.834 Var:4%
http://vsnet.aerith.net/misao/data/MisV/MisV1149.gif
MisV1149 20001013.60477 11.88C Mis KAF-1600 Tycho_Catalogue Akira_Takao 200-mm_f/4_camera_lens_+_SBIG_ST-8
MisV1149 20001224.37968 10.97C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1149 20001224.38154 10.95C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1149 20001224.38339 10.97C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1149 20001224.38524 10.98C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1149 20010727.76395 11.20C Mis KAF-1600 Tycho_Catalogue Akira_Takao 200-mm_f/4_camera_lens_+_SBIG_ST-8
MisV1149 20011010.58640 10.74C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1149 20011010.58838 10.70C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
MisV1149 20011010.59035 10.77C Mis KAF-1600 Tycho_Catalogue Nobuo_Ohkura 500-mm_camera_lens_+_SBIG_ST-8
Seiichi Yoshida, MISAO Project; Akira Takao, Kita Kyushu, Fukuoka,
Japan; and KenIchi Kadota, MISAO Project, discovered a new variable
star MisV1149.
It was picked up by Seiichi Yoshida from the candidates of new
variable stars detected by the PIXY system 2 from images taken by
Akira Takao, and confirmed by KenIchi Kadota.
The identification is researched by Taichi Kato (Kyoto University),
John Greaves (the United Kingdom), and Seiichi Yoshida.
The magnitude are measured automatically by the PIXY system 2.
About the MISAO Project and the PIXY system 2:
http://vsnet.aerith.net/misao/
--
Seiichi Yoshida
comet@aerith.net
http://vsnet.aerith.net/
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