
Home Page Updated on December 16, 2020
MisV1073
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| R.A. | 20h01m44s.24 | |
| Decl. | +46o58'20".8 | (2000.0) |
| Mag. | 11.3-11.8C | |
| Type | SR: |
= USNO-A2.0 1350.11491324 20h01m44s.228 +46o58'21".44 Mag(R):13.6 M ag(B):15.8 = IRAS 20001+4649 20h01m42s.6 +46o58'21" Ellipse:38x9" P.A.:65 Flu x(12):0.3021 Flux(25):<0.2500 Flux(60):<0.5274 Flux(100):<42.48 = 2MASS 200144.208 +465820.68 (2000.0) 7.980 6.940 6.539
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 MisV1073.
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 comparing with images taken by Ken-ichi Kadota, and confirmed by Ken-ichi Kadota.
The identification is researched by Taichi Kato (Kyoto University), John Greaves (the United Kingdom), and Seiichi Yoshida.
John Greaves pointed out that there is an X-ray star 1RXS 200142.7+465727 about 1 arcmin south of MisV1073. But they are probably not the same because of the large distance.
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11.9 +--------------------------------------------------------+
2451273 2451853
1999 Apr. 4 2000 Nov. 4
| Date | Mag | Filter | Observer |
|---|---|---|---|
| 1999 Apr. 30.68128 | 11.6 | C | Ken-ichi Kadota |
| 1999 Apr. 30.68170 | 11.6 | C | Ken-ichi Kadota |
| 1999 July 24.60014 | 11.3 | C | Ken-ichi Kadota |
| 1999 July 24.60056 | 11.3 | C | Ken-ichi Kadota |
| 2000 Sept. 17.44029 | 11.8 | C | Nobuo Ohkura |
| 2000 Sept. 17.44214 | 11.8 | C | Nobuo Ohkura |
| 2000 Sept. 17.44399 | 11.8 | C | Nobuo Ohkura |
| 2000 Oct. 9.41291 | 11.7 | C | Nobuo Ohkura |
| 2000 Oct. 9.41475 | 11.6 | C | Nobuo Ohkura |
| 2000 Oct. 9.41661 | 11.5 | C | Nobuo Ohkura |