Home Page Updated on December 16, 2020
MisV1032
|
R.A. | 20h42m15s.85 | |
Decl. | +45o32'50".4 | (2000.0) |
Mag. | 10.8-14.5C | |
Type | M? |
= USNO-A2.0_1350.12776036 20 42 15.853 +45 32 50.41 13.5R 19.6B = IRAS 20405+4521 R.A.=20 42 16.19 Decl.=+45 32 48.0 (7 x 7", p.a.= 123) flux(12)=13.73 flux(25)=8.93 flux(60)=<1.85 flux(100)=<17.3 7 77% variable = 2MASS 204215.816 +453249.67 (2000.0) 5.940 0.000 0.000
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 MisV1032.
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.
10.5 +--------------------------------------------------------+ | * | | * | | | | | | | | | | v | | | | | | | | | | | | | | | | v | | | | v | | * | | * | | * * | | * | 14.7 +--------------------------------------------------------+ 2450392 2451890 1996 Nov. 4 2000 Dec. 11
Date | Mag | Filter | Observer |
---|---|---|---|
1997 Jan. 11.43951 | 14.0 | C | Masayuki Suzuki |
1997 Jan. 11.44507 | [11.8 | C | Masayuki Suzuki |
1997 Jan. 15.38657 | [13.3 | C | Masayuki Suzuki |
1997 Jan. 15.38829 | [13.7 | C | Masayuki Suzuki |
1999 July 9.76147 | 14.3 | C | Ken-ichi Kadota |
1999 July 9.76243 | 14.2 | C | Ken-ichi Kadota |
1999 Nov. 21.46437 | 14.5 | C | Ken-ichi Kadota |
1999 Nov. 21.46480 | 14.3 | C | Ken-ichi Kadota |
2000 Aug. 13.50325 | 10.8 | C | Nobuo Ohkura |
2000 Aug. 13.50510 | 10.8 | C | Nobuo Ohkura |
2000 Oct. 4.44953 | 10.7 | C | Nobuo Ohkura |
2000 Oct. 4.45140 | 10.7 | C | Nobuo Ohkura |
2000 Oct. 4.45325 | 10.7 | C | Nobuo Ohkura |