Home Page Updated on December 16, 2020
MisV0910
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| R.A. | 17h02m57s.47 | |
| Decl. | -28o57'18".4 | (2000.0) |
| Mag. | 11.3-12.3C | |
| Type | SR: |
= USNO-A2.0_0600.23329190 17 02 57.467 -28 57 18.41 13.3R 16.6B
Digitized Sky Survey GIF image (15 x 15 arcmin)
NSVS Light Curve (NSVS 19311996)
Discovery Information
Seiichi Yoshida, MISAO Project; and Ken-ichi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV0910.
It was detected by the PIXY system as one of the candidates of new variable stars from images taken by Kadota, then confirmed by Yoshida.
MisV0909 is 19 arcsec to the east of MisV0910. The brightness of these two stars reversed between 1999 April and 2000 February.
Special Notes
A pair of double variable stars with 19 arcsec distance.
Light Curve
11.3 +--------------------------------------------------------+
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12.4 +--------------------------------------------------------+
2451267 2451615
1999 Mar. 29 2000 Mar. 11
Observations by MISAO Project
| Date | Mag | Filter | Observer |
|---|---|---|---|
| 1999 Apr. 14.72459 | 12.3 | C | Ken-ichi Kadota |
| 1999 Apr. 14.72521 | 12.0 | C | Ken-ichi Kadota |
| 1999 Aug. 1.49862 | 11.8 | C | Ken-ichi Kadota |
| 1999 Aug. 1.49905 | 11.9 | C | Ken-ichi Kadota |
| 2000 Feb. 24.81190 | 11.3 | C | Ken-ichi Kadota |
| 2000 Feb. 24.81247 | 11.3 | C | Ken-ichi Kadota |