
Home Page Updated on December 16, 2020
MisV0395
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| R.A. | 17h56m57s.17 | |
| Decl. | -18o52'12".6 | (2000.0) |
| Mag. | 13.2-[14.2C | |
| Type | SR? |
= IRAS 17540-1851 R.A.=17 56 56.86 Decl.=-18 52 13.8 (21 x 5", p.a.
=90) flux(12)=7.50 flux(25)=2.97 flux(60)=<7.22 flux(100)=<70.83
88% variable
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.
Taichi Kato pointed out that the photometry of this object was obtained as NGC 6194 No. 1130 and this is a red star.
Taichi Kato revealed that it was observed as NGC 6194 No. 1130 and is a red star.
13.2 +--------------------------------------------------------+
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14.3 +--------------------------------------------------------+
2451270 2451429
1999 Apr. 1 1999 Sept. 7
| Date | Mag | Filter | Observer |
|---|---|---|---|
| 1999 Apr. 8.74416 | 13.3 | C | Ken-ichi Kadota |
| 1999 Apr. 8.74471 | 13.2 | C | Ken-ichi Kadota |
| 1999 Apr. 30.75339 | 13.5 | C | Ken-ichi Kadota |
| 1999 Apr. 30.75384 | 13.5 | C | Ken-ichi Kadota |
| 1999 Aug. 31.55559 | [14.2 | C | Ken-ichi Kadota |
| 1999 Aug. 31.55602 | 14.2 | C | Ken-ichi Kadota |