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[vsnet-newvar 449] New variable star MisV0931
- Date: Wed, 14 Jun 2000 21:57:37 -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 449] New variable star MisV0931
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues,
New variable star discovery by the MISAO Project (MisV0931).
MisV0931
R.A. 19h42m03s.78
Decl. +10o41'33".1 (2000.0)
Mag. 11.9C-14.7C
Type ?
= USNO-A2.0_0975.16058104 19 42 03.777 +10 41 33.13 14.4R 17.3B
= IRAS 19396+1034 R.A.=19 42 03.58 Decl.=+10 41 31.0 (28 x 7", p.a.=76) flux(12)=4.68 flux(25)=2.62 flux(60)=0.57 flux(100)=<10.25 87% variable
http://vsnet.aerith.net/misao/data/MisV/MisV0931.gif
MisV0931 19990715.61310 119C Mis image="KenIchi Kadota"
MisV0931 20000505.65618 147C Mis image="Nobuo Ohkura"
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV0931.
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".
Taichi Kato pointed out that the spectral type is M10III (Buscombe W.,
"Twelveth General Catalogue of MK Spectral Classification",
Northwestern Univ., Evanston, Illinois, 1995).
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