Home Page Updated on December 16, 2020
MisV1034
|
R.A. | 21h07m49s.77 | |
Decl. | +46o03'00".5 | (2000.0) |
Mag. | 12.1-13.1C |
= IRAS 21060+4550 R.A.=21 07 50.29 Decl.=+46 03 03.9 (31 x 4", p.a. =51) flux(12)=7.36 flux(25)=2.98 flux(60)=0.92 flux(100)=<4.26 29% 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 MisV1034.
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.
Taichi Kato and John Greaves pointed out this object is identified with a carbon star CS5158.
12.0 +--------------------------------------------------------+ | * | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | * | | | | * | | | | * | 13.2 +--------------------------------------------------------+ 2451491 2451784 1999 Nov. 8 2000 Aug. 27
Date | Mag | Filter | Observer |
---|---|---|---|
1999 Nov. 21.50859 | 12.1 | C | Ken-ichi Kadota |
1999 Nov. 21.50907 | 12.1 | C | Ken-ichi Kadota |
2000 Aug. 14.50396 | 13.0 | C | Nobuo Ohkura |
2000 Aug. 14.50581 | 12.9 | C | Nobuo Ohkura |
2000 Aug. 14.50766 | 13.1 | C | Nobuo Ohkura |