
Home Page Updated on February 28, 2013
MisV0078
|
| R.A. | 18h06m26s.93 | |
| Decl. | -27o29'21".2 | (2000.0) |
| Mag. | 13.1-16.5Rc | |
| Type | M | |
| Period | 272.4 | |
| Epoch | 2451278.0 |
= USNO0600.15154453 18 06 26.931 -27 29 21.17 16.2R 16.8B
Digitized Sky Survey GIF image (15 x 15 arcmin)
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.
Stefan Huemmerich and Klaus Bernhard revealed that it is a Mira type variable with a period of 272.4 days, brightness range of 13.1-16.5 mag(Rc), using the MACHO project data (light curve, phase diagram).


| Date | Mag | Filter | Observer |
|---|---|---|---|
| 1999 May 7.73164 | 14.3 | C | Ken-ichi Kadota |
| 1999 May 7.73260 | 14.5 | C | Ken-ichi Kadota |
| 1999 June 12.61597 | 15.2 | C | Ken-ichi Kadota |