
Home Page Updated on December 16, 2020
MisV0990
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| R.A. | 19h40m54s.86 | |
| Decl. | +18o21'15".2 | (2000.0) |
| Mag. | 12.1-13.1C | |
| Type | SR? |
= IRAS 19386+1814 R.A.=19 40 55.10 Decl.=+18 21 15.8 (27 x 5", p.a.
=71) flux(12)=1.52 flux(25)=0.62 flux(60)=<0.57 flux(100)=<30.68
95% variable
= 2MASS 194054.848 +182114.58 (2000.0) 6.685 5.660 5.117
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 MisV0990.
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.
12.0 +--------------------------------------------------------+
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13.2 +--------------------------------------------------------+
2451359 2451706
1999 June 29 2000 June 10
| Date | Mag | Filter | Observer |
|---|---|---|---|
| 1999 July 15.63538 | 13.1 | C | Ken-ichi Kadota |
| 1999 July 15.63604 | 13.0 | C | Ken-ichi Kadota |
| 2000 May 25.66708 | 12.3 | C | Nobuo Ohkura |
| 2000 May 25.66894 | 12.1 | C | Nobuo Ohkura |