Home Page Updated on December 16, 2020
MisV0909
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| R.A. | 17h02m58s.92 | |
| Decl. | -28o57'15".6 | (2000.0) |
| Mag. | 11.2-12.1C | |
| Type | SR: |
= USNO-A2.0_0600.23332867 17 02 58.919 -28 57 15.56 12.6R 16.8B
Digitized Sky Survey GIF image (15 x 15 arcmin)
Discovery Information
Seiichi Yoshida, MISAO Project; and Ken-ichi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV0909.
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.
MisV0910 is 19 arcsec to the west of MisV0909. 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
11.1 +--------------------------------------------------------+
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12.2 +--------------------------------------------------------+
2451267 2451615
1999 Mar. 29 2000 Mar. 11
Observations by MISAO Project
| Date | Mag | Filter | Observer |
|---|---|---|---|
| 1999 Apr. 14.72459 | 11.2 | C | Ken-ichi Kadota |
| 1999 Apr. 14.72521 | 11.2 | C | Ken-ichi Kadota |
| 1999 Aug. 1.49862 | 11.5 | C | Ken-ichi Kadota |
| 1999 Aug. 1.49905 | 11.5 | C | Ken-ichi Kadota |
| 2000 Feb. 24.81190 | 12.1 | C | Ken-ichi Kadota |
| 2000 Feb. 24.81247 | 12.1 | C | Ken-ichi Kadota |