Home Page Updated on December 16, 2020
MisV1031
|
R.A. | 20h38m19s.74 | |
Decl. | +34o12'20".3 | (2000.0) |
Mag. | 11.4-13.6C | |
Type | M? |
= IRAS 20363+3401 R.A.=20 38 19.81 Decl.=+34 12 21.3 (24 x 5", p.a. =63) flux(12)=6.21 flux(25)=5.10 flux(60)=0.68 flux(100)=<36.21 99% variable = 2MASS 203819.812 +341220.71 (2000.0) 7.216 5.992 5.095
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 MisV1031.
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.
11.3 +--------------------------------------------------------+ | * | | * | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | * | 13.7 +--------------------------------------------------------+ 2451350 2451780 1999 June 20 2000 Aug. 23
Date | Mag | Filter | Observer |
---|---|---|---|
1999 July 9.77422 | 13.6 | C | Ken-ichi Kadota |
1999 July 9.77470 | 13.6 | C | Ken-ichi Kadota |
2000 Aug. 3.54104 | 11.4 | C | Nobuo Ohkura |
2000 Aug. 3.54289 | 11.5 | C | Nobuo Ohkura |