
Home Page Updated on February 28, 2013
MisV0314
|
| R.A. | 17h00m14s.94 | |
| Decl. | -21o01'28".2 | (2000.0) |
| Mag. | 12.2-13.4C |
= USNO-A2.0_0675.17367497 17 00 14.941 -21 01 28.19 13.9R 16.3B
Digitized Sky Survey GIF image (15 x 15 arcmin)
NSVS Light Curve (NSVS 19262533)
NSVS Light Curve (NSVS 16450628)
NSVS Light Curve (NSVS 16449274)
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.
V1191 Oph is 66.5 arcsec from MisV0314. No star brighter than 15.3C mag was detected at the position of V1191 Oph. However, considering the large distance, MisV0314 is probably another new variable object.
12.1 +--------------------------------------------------------+
| * |
| |
| * |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| |
| * |
13.5 +--------------------------------------------------------+
2451278 2451397
1999 Apr. 9 1999 Aug. 6
| Date | Mag | Filter | Observer |
|---|---|---|---|
| 1999 Apr. 14.71407 | 13.4 | C | Ken-ichi Kadota |
| 1999 Apr. 14.71463 | 13.4 | C | Ken-ichi Kadota |
| 1999 Aug. 1.51620 | 12.3 | C | Ken-ichi Kadota |
| 1999 Aug. 1.51757 | 12.2 | C | Ken-ichi Kadota |