Home Page Updated on December 16, 2020
MisV1237
|
R.A. | 01h03m28s.90 | |
Decl. | +43o01'27".6 | (2000.0) |
Mag. | 13.34-13.94C | |
Type | EA | |
Period | 7.5530 | |
Epoch | 2453598.1280 |
= GSC 2807-01148 01h03m28s.90 +43o01'27".6 Error:0.2" Mag:13.32 Ma gError:0.28 Band:6 Class:0 Plate:02RY Flag:F Epoch:04 AUG 1984 = USNO-A2.0 1275.00629576 01h03m28s.869 +43o01'27".77 Mag(R):13.3 M ag(B):13.9
Digitized Sky Survey GIF image (15 x 15 arcmin)
NSVS Light Curve (NSVS 3804047)
Seiichi Yoshida, MISAO Project; Nobuo Ohkura, Okayama, Japan; and Ken-ichi Kadota, MISAO Project, discovered a new variable star MisV1237.
It was picked up by Seiichi Yoshida from the candidates of new variable stars detected by the PIXY system 2 from images taken by Nobuo Ohkura, and confirmed by Ken-ichi Kadota.
The identification is researched by Taichi Kato (Kyoto University), Seiichi Yoshida, and other contributors.
Kazuhiro Nakajima's observations revealed it is an Algol-type (EA) eclipsing variable with unfiltered CCD variations of 13.34 mag at maximum, 13.94 mag at primary minimum, 13.90 mag at secondary minimum, and period of 7.5530 days (IBVS 5700).
Our second eccentric binary. The secondary minimum occurs at the phase of 0.484.
Date | Mag | Filter | Observer |
---|---|---|---|
2000 Dec. 14.43639 | 13.13 | C | Nobuo Ohkura |
2000 Dec. 14.43823 | 13.18 | C | Nobuo Ohkura |
2000 Dec. 14.44009 | 13.21 | C | Nobuo Ohkura |
2001 Oct. 18.58205 | 13.27 | C | Nobuo Ohkura |
2001 Oct. 18.58403 | 13.12 | C | Nobuo Ohkura |
2001 Oct. 29.53333 | 13.91 | C | Nobuo Ohkura |
2001 Oct. 29.53530 | 13.83 | C | Nobuo Ohkura |
2001 Dec. 7.44898 | 13.19 | C | Nobuo Ohkura |
2001 Dec. 7.45096 | 13.19 | C | Nobuo Ohkura |
2001 Dec. 16.41515 | 13.33 | C | Nobuo Ohkura |
2001 Dec. 16.41612 | 13.30 | C | Nobuo Ohkura |
2001 Dec. 18.41396 | 13.17 | C | Nobuo Ohkura |
2001 Dec. 18.41593 | 13.24 | C | Nobuo Ohkura |