Home Page Updated on December 16, 2020
MisV0880
|
| R.A. | 18h02m57s.75 | |
| Decl. | -28o11'53".2 | (2000.0) |
| Mag. | 11.2:-15.4Rc | |
| Type | M | |
| Period | 222.6 | |
| Epoch | 2451389.0 |
Digitized Sky Survey GIF image (15 x 15 arcmin)
NSVS Light Curve (NSVS 19382447)
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.
Special Notes
Stefan Huemmerich and Klaus Bernhard revealed that it is a Mira type variable with a period of 222.6 days, brightness range of 11.2:-15.4 mag(Rc), using the MACHO project data.
Light Curve
12.7 +--------------------------------------------------------+
| * |
| |
| * |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| * |
| |
| |
| |
| |
| |
| * |
14.2 +--------------------------------------------------------+
2451437 2451607
1999 Sept. 15 2000 Mar. 3
Observations by MISAO Project
| Date | Mag | Filter | Observer |
|---|---|---|---|
| 1999 Sept. 23.43274 | 14.1 | C | Ken-ichi Kadota |
| 1999 Sept. 23.43324 | 13.7 | C | Ken-ichi Kadota |
| 2000 Feb. 24.83672 | 12.8 | C | Ken-ichi Kadota |
| 2000 Feb. 24.83728 | 12.9 | C | Ken-ichi Kadota |