Home Page Updated on December 16, 2020
MisV0850
|
| R.A. | 18h02m03s.69 | |
| Decl. | -32o38'32".7 | (2000.0) |
| Mag. | 12.8-14.5C | |
| Type | SR? |
= 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)
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 +--------------------------------------------------------+
| * |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| * |
| |
| |
| |
| |
| * |
14.6 +--------------------------------------------------------+
2451305 2451613
1999 May 6 2000 Mar. 9
Observations by MISAO Project
| Date | Mag | Filter | Observer |
|---|---|---|---|
| 1999 May 20.68679 | 12.8 | C | Ken-ichi Kadota |
| 1999 May 20.68723 | 12.8 | C | Ken-ichi Kadota |
| 2000 Feb. 24.84394 | 14.5 | C | Ken-ichi Kadota |
| 2000 Feb. 24.84450 | 14.1 | C | Ken-ichi Kadota |