Home Page Updated on December 16, 2020
MisV0348
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| R.A. | 18h00m52s.25 | |
| Decl. | -28o10'51".4 | (2000.0) |
| Mag. | 12.0-15.7Rc | |
| Type | M | |
| Period | 163.8 | |
| Epoch | 2451245.0 |
= USNO-A2.0_0600.29966820 18 00 52.254 -28 10 51.42 16.6R 18.5B
Digitized Sky Survey GIF image (15 x 15 arcmin)
Discovery Information
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.
V1002 Sgr is 1.7 arcmin from MisV0348. But this is another variable star.
Special Notes
Stefan Huemmerich and Klaus Bernhard revealed that it is a Mira type variable with a period of 163.8 days, brightness range of 12.0-15.7 mag(Rc), using the MACHO project data.
Research and Publication
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New Variable Stars Discovered in the MISAO Project VI: MisV0301-MisV0350
IBVS 4812
Yoshida, S.; Kadota, K.; Kato, T.
Light Curve
13.1 +--------------------------------------------------------+
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14.2 +--------------------------------------------------------+
2451276 2451300
1999 Apr. 7 1999 May 1
Observations by MISAO Project
| Date | Mag | Filter | Observer |
|---|---|---|---|
| 1999 Apr. 8.75605 | 13.1 | C | Ken-ichi Kadota |
| 1999 Apr. 8.75661 | 13.3 | C | Ken-ichi Kadota |
| 1999 Apr. 30.74204 | 14.1 | C | Ken-ichi Kadota |