Home Page Updated on April 20, 2018
MisV0740
|
R.A. | 17h59m41s.66 | |
Decl. | -00o35'31".0 | (2000.0) |
Mag. | 12.9-14.7C | |
Type | SR: |
= USNO-A2.0_0825.11686444 17 59 41.657 -00 35 30.97 15.5R 17.1B = IRAS 17571-0035 R.A.=17 59 44.12 Decl.=-00 35 47.8 (38 x 8", p.a. =87) flux(12)=0.51 flux(25)=<0.25 flux(60)=<0.40 flux(100)=<1.95
Digitized Sky Survey GIF image (15 x 15 arcmin)
It was detected by the PIXY system as one of the candidates of new variable stars from images taken by Ken-ichi Kadota, Ageo City, Saitama, Japan, then confirmed by Seiichi Yoshida.
TASS J175944.6-003558 is 50 arcsec from MisV0740. TASS J175944.6-003558 was detected as another variable star between 11.7 and 14.2 mag. Therefore, MisV0740 is another new variable star.
Date | Mag | Filter | Observer |
---|---|---|---|
1999 Apr. 14.73889 | 12.9 | C | Ken-ichi Kadota |
1999 Apr. 14.73932 | 12.9 | C | Ken-ichi Kadota |
1999 July 15.54193 | 14.3 | C | Ken-ichi Kadota |
1999 July 15.54241 | 14.4 | C | Ken-ichi Kadota |
1999 Aug. 1.54603 | 14.7 | C | Ken-ichi Kadota |
1999 Aug. 1.54676 | 14.6 | C | Ken-ichi Kadota |