[vsnet-newvar 32] New variable star MisV0696

[Seiichi Yoshida <seiichi@muraoka.info.waseda.ac.jp>]

Dear colleagues,

New variable star discovery by the MISAO Project (MisV0696).

MisV0696
  R.A.  19h02m36s.04
  Decl. -01o06'17".0  (2000.0)
  Mag.  12.6C-14.2C
  Type  ?
= USNO-A2.0_0825.14163260  19 02 36.036  -01 06 17.02  13.0R  16.3B

  http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/misao/data/MisV/MisV0696.gif

MisV0696 19990414.75911 126C Mis
MisV0696 19990414.75954 126C Mis
MisV0696 19990508.71193 129C Mis
MisV0696 19990508.71236 130C Mis
MisV0696 19990724.51391 141C Mis
MisV0696 19990724.51481 142C Mis

It was detected by the PIXY system as one of the candidates of new
variable stars from images taken by KenIchi Kadota, Ageo City,
Saitama, Japan, then confirmed by Seiichi Yoshida.

NSV 11675 is 2.7 arcmin from MisV0696. No star brighter than 14.2 mag
was detected at the catalogued position on our unfiltered CCD images.
However, considering the large distance, MisV0696 is probably another
new variable object.

HS 1411, one of the variable stars discovered by FASTT, Flagstaff
Astrometric Scanning Transit Telescope, is 1.2 arcmin from MisV0696. 
HS 1411 was detected as another variable star between 10.8 and 11.4
mag. Therefore, MisV0696 is another new variable star.

Please see the URL below for the MISAO Project and the PIXY system.

  http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/misao/

--
Seiichi Yoshida
seiichi@muraoka.info.waseda.ac.jp
http://vsnet.info.waseda.ac.jp/muraoka/members/seiichi/index.html

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