Home Page Updated on December 16, 2020
MisV1030
|
R.A. | 20h31m21s.00 | |
Decl. | +33o36'46".8 | (2000.0) |
Mag. | 12.4-13.8C |
= USNO-A2.0_1200.15249451 20 31 20.995 +33 36 46.75 14.5R 17.4B = IRAS 20293+3326 R.A.=20 31 21.64 Decl.=+33 36 49.4 (23 x 9", p.a. =68) flux(12)=0.97 flux(25)=0.51 flux(60)=<1.60 flux(100)=<79.05 93% variable
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 MisV1030.
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.
12.3 +--------------------------------------------------------+ | * | | * | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | * | | * | 13.9 +--------------------------------------------------------+ 2451314 2451781 1999 May 15 2000 Aug. 24
Date | Mag | Filter | Observer |
---|---|---|---|
1999 June 5.74081 | 13.7 | C | Ken-ichi Kadota |
1999 June 5.74134 | 13.8 | C | Ken-ichi Kadota |
2000 Aug. 3.53734 | 12.4 | C | Nobuo Ohkura |
2000 Aug. 3.53919 | 12.5 | C | Nobuo Ohkura |