Home Page Updated on December 16, 2020
MisV1019
|
R.A. | 21h12m04s.74 | |
Decl. | +39o24'10".8 | (2000.0) |
Mag. | 12.1-14.1C | |
Type | SR? |
= 2MASS 211204.632 +392415.48 (2000.0) 0.000 0.000 0.000 = 2MASS 211204.733 +392410.62 (2000.0) 7.285 6.198 5.577
Digitized Sky Survey GIF image (15 x 15 arcmin)
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and Ken-ichi Kadota, Ageo, Saitama, Japan, discovered a new variable star MisV1019.
It was picked up by Yoshida from the candidates of new variable stars detected by the PIXY system from images taken by Ohkura comparing with images taken by Kadota. Kadota and Yoshida judged it as a real variable star.
The identification with the 2MASS data is by Taichi Kato.
12.0 +--------------------------------------------------------+ | * | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | * | 14.2 +--------------------------------------------------------+ 2451492 2451764 1999 Nov. 9 2000 Aug. 7
Date | Mag | Filter | Observer |
---|---|---|---|
1999 Nov. 21.49338 | 14.1 | C | Ken-ichi Kadota |
1999 Nov. 21.49383 | 14.1 | C | Ken-ichi Kadota |
2000 July 26.57524 | 12.1 | C | Nobuo Ohkura |
2000 July 26.57709 | 12.1 | C | Nobuo Ohkura |