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[vsnet-newvar 615] New variable star MisV1024

Dear colleagues,

New variable star discovery by the MISAO Project (MisV1024).

MisV1024
  R.A.  20h01m35s.73
  Decl. +33o59'03".4  (2000.0)
  Mag.  12.2C-13.0C
  Type  SR?
= IRAS 19596+3350  R.A.=20 01 35.88  Decl.=+33 59 04.6  (19 x 3", p.a.=66)  flux(12)=1.07  flux(25)=0.47  flux(60)=<3.73  flux(100)=<60.10  19% variable
= 2MASS 200135.610 +335902.75 (2000.0)  7.312  5.861  6.583

  http://vsnet.aerith.net/misao/data/MisV/MisV1024.gif

MisV1024 19990430.69576 129C Mis image="KenIchi Kadota"
MisV1024 19990430.69619 129C Mis image="KenIchi Kadota"
MisV1024 19990707.68187 122C Mis image="KenIchi Kadota"
MisV1024 19990707.68231 122C Mis image="KenIchi Kadota"
MisV1024 19990801.60674 126C Mis image="KenIchi Kadota"
MisV1024 19990801.60715 126C Mis image="KenIchi Kadota"
MisV1024 19990803.65993 126C Mis image="KenIchi Kadota"
MisV1024 19990803.66037 126C Mis image="KenIchi Kadota"
MisV1024 19990831.63432 128C Mis image="KenIchi Kadota"
MisV1024 19990831.63475 128C Mis image="KenIchi Kadota"
MisV1024 20000803.51880 130C Mis image="Nobuo Ohkura"
MisV1024 20000803.52065 128C Mis image="Nobuo Ohkura"

Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and
KenIchi Kadota, Ageo, Saitama, Japan, discovered a new variable star
MisV1024.

It was picked up by Yoshida from the candidates of new variable stars
detected by the PIXY system from images taken by Ohkura comparing with
images taken by Kadota. Kadota and Yoshida judged it as a real
variable star.

The magnitude are measured automatically by the PIXY system. Image
observers' names are noted after "Mis".

Taichi Kato pointed out that this object is identified with a S-type
star NSS 49.

The identification with the 2MASS data is by Taichi Kato.

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/

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