MISAO Project

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* Profile

MisV0850

R.A.18h02m03s.69
Decl.-32o38'32".7(2000.0)
Mag.12.8-14.5C
TypeSR?
= IRAS 17588-3238  R.A.=18 02 05.73  Decl.=-32 38 37.0  (70 x 11", p.a
  .=92)  flux(12)=0.55  flux(25)=<0.78  flux(60)=<4.08  flux(100)=<41.
  08

Digitized Sky Survey GIF image (15 x 15 arcmin)

SIMBAD Query

AAVSO VSX Database

ASAS-3 Light Curve

* Discovery Information

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

NSV 09990 is 2.6 arcmin from MisV0850. No star brighter than 14.5 mag was detected at the cataloged position of NSV 09990. But considering the large angular distance and the magnitude of NSV 09990 (15.3 - 16 mag) in the catalog, MisV0850 is probably a new variable star.

* Light Curve

    12.7  +--------------------------------------------------------+
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    14.6  +--------------------------------------------------------+
       2451305                                                  2451613
     1999 May 6                                               2000 Mar. 9

* Observations by MISAO Project

DateMagFilterObserver
1999 May 20.6867912.8CKen-ichi Kadota
1999 May 20.6872312.8CKen-ichi Kadota
2000 Feb. 24.8439414.5CKen-ichi Kadota
2000 Feb. 24.8445014.1CKen-ichi Kadota

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