
Home Page Updated on August 27, 2010
MisV1339
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| R.A. | 03h04m34s.90 | |
| Decl. | +57o09'35".0 | (2000.0) |
| Mag. | 10.02-10.27C | |
| Type | SR: |
= GSC 3709-00631 03h04m34s.82 +57o09'35".6 Error:0.3" Mag:9.75 Mag Error:0.40 Band:1 Class:0 Plate:036E Flag:T Epoch:11 OCT 1983 = GSC 3709-00631 03h04m34s.96 +57o09'34".6 Error:0.3" Mag:10.02 Ma gError:0.40 Band:1 Class:0 Plate:01W1 Flag:T Epoch:04 NOV 1983 = USNO-A2.0 1425.04109032 03h04m34s.885 +57o09'35".17 Mag(R):10.3
Digitized Sky Survey GIF image (15 x 15 arcmin)
2MASS Quicklook Image (5 x 5 arcmin)
NSVS Light Curve (NSVS 1942992)
Kazuhiro Nakajima, Mie, Japan, discovered a new variable star MisV1339.
It was picked up during time series photometry of MisV1317 in the course of the MISAO Project.
The light curve suggests it is a semi regular variable with an unfiltered CCD amplitude of 0.25 mag between 10.02 - 10.27 mag.
Not only the long term variation, a short term oscillation with an amplitude of 0.10 mag was also confirmed by the time series photometry on three nights.
MisV1339 is almost constant at 10.323 +/- 0.022 mag in the NSVS data.
Discovered during time series photometry of MisV1317.
The light curve suggests it is a semi regular variable with an unfiltered CCD amplitude of 0.25 mag between 10.02 - 10.27 mag.
Not only the long term variation, a short term oscillation with an amplitude of 0.10 mag was also confirmed by the time series photometry on three nights in the course of Kazuhiro Nakajima's observations.
MisV1339 is almost constant at 10.323 +/- 0.022 mag in the NSVS data.
Michael Richmond researched the TASS Mark IV database and found one feature in the I-band, but otherwise no obvious variations was found (light curve). The mean color is (V-I) = 0.79.
Mitsugu Fujii's spectrum on 2008 Mar. 5 (the red is MisV1339) is a normal spectrum of a G-type star.




| Date | Mag | Filter | Observer |
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