Home Page Updated on December 16, 2020
MisV0796
|
| R.A. | 18h00m30s.43 | |
| Decl. | -27o23'42".2 | (2000.0) |
| Mag. | 12.7-16.4Rc | |
| Type | M | |
| Period | 298 | |
| Epoch | 2450980 |
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.
Special Notes
Klaus Bernhard and Stefan Huemmerich reported the MACHO data revealed it is a Mira type variable with a period of 298 days, brightness range of 12.7-16.4 mag(Rc) (light curve).
Light Curve
Observations by MISAO Project
| Date | Mag | Filter | Observer |
|---|---|---|---|
| 1999 Apr. 8.75605 | 12.1 | C | Ken-ichi Kadota |
| 1999 Apr. 8.75661 | 12.1 | C | Ken-ichi Kadota |
| 1999 June 4.62189 | 12.6 | C | Ken-ichi Kadota |
| 1999 June 4.62278 | 12.6 | C | Ken-ichi Kadota |
| 1999 June 4.62519 | 12.9 | C | Ken-ichi Kadota |
| 1999 Sept. 23.43172 | 13.9 | C | Ken-ichi Kadota |
| 1999 Sept. 23.43219 | 13.8 | C | Ken-ichi Kadota |