
Home Page Updated on December 16, 2020
MisV0301
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| R.A. | 19h01m27s.60 | |
| Decl. | +20o57'28".4 | (2000.0) |
| Mag. | 13.7-15.0C |
= USNO-A2.0_1050.12612555 19 01 27.604 +20 57 28.37 16.0R 19.4B = IRAS 18592+2053 R.A.=19 01 26.96 Decl.=+20 57 23.0 (57 x 8", p.a. =77) flux(12)=0.39 flux(25)=<0.25 flux(60)=<0.40 flux(100)=<10.0 0
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.
Diego Rodriguez observed its slow fading in 2010 summer, and pointed out that it is a possible Mira variable.
13.6 +--------------------------------------------------------+
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15.1 +--------------------------------------------------------+
2451296 2451397
1999 Apr. 27 1999 Aug. 6
2010 Sept.21.866 15.24 CR Diego Rodriguez 2010 Sept. 8.892 15.26 CR Diego Rodriguez 2010 July 29.916 14.46 CR Diego Rodriguez 2010 July 5.920 14.40 CR Diego Rodriguez 2010 June 27.922 14.41 CR Diego Rodriguez
| Date | Mag | Filter | Observer |
|---|---|---|---|
| 1999 May 1.71324 | 13.9 | C | Ken-ichi Kadota |
| 1999 May 1.71380 | 13.7 | C | Ken-ichi Kadota |
| 1999 Aug. 1.57221 | 15.0 | C | Ken-ichi Kadota |
| 1999 Aug. 1.57285 | 14.9 | C | Ken-ichi Kadota |