Home Page Updated on December 16, 2020
MisV0871
|
R.A. | 18h01m06s.63 | |
Decl. | -27o41'25".8 | (2000.0) |
Mag. | 11.6:-16.5Rc | |
Type | M | |
Period | 255 | |
Epoch | 2450533 |
= USNO-A2.0_0600.29987534 18 01 06.941 -27 41 33.73 13.2R 15.5B
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.
Klaus Bernhard and Stefan Huemmerich reported the MACHO data revealed it is a Mira type variable with a period of 255 days, brightness range of 11.6:-16.5 mag(Rc) (light curve).
Date | Mag | Filter | Observer |
---|---|---|---|
1999 Apr. 8.75605 | 11.8 | C | Ken-ichi Kadota |
1999 Apr. 8.75661 | 11.9 | C | Ken-ichi Kadota |
1999 Apr. 30.74204 | 12.2 | C | Ken-ichi Kadota |
2000 Feb. 24.83672 | 13.4 | C | Ken-ichi Kadota |
2000 Feb. 24.83728 | 13.5 | C | Ken-ichi Kadota |