Multisite photometric campaign on the high-amplitude δ Scuti star KIC 6382916
نویسندگان
چکیده
منابع مشابه
The first high-amplitude δ Scuti star in an eclipsing binary system
We report the discovery of the first high-amplitude δ Scuti star in an eclipsing binary, which we have designated UNSW-V-500. The system is an Algol-type semi-detached eclipsing binary of maximum brightness V = 12.52 mag. A best-fitting solution to the binary light curve and two radial velocity curves is derived using the Wilson–Devinney code. We identify a late-A spectral-type primary componen...
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An order-of-magnitude estimate for the incidence of high-amplitude δ Scuti-type variable stars (HADS) in the δ Scuti area of the H-R diagram is calculated. Using a model for the stellar distribution in the Milky Way, we calculate the number of stars that are expected to fall in the δ Scuti area of the H-R diagram within the magnitude range and sky coverage of the ROTSE Survey for Variables I (R...
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We present yb time–series CCD photometry of the high–amplitude δ Scuti star V 1162 Ori. A period break and a significant decrease in amplitude (50 percent) has been reported for this star by Hintz et al. (1998). New observations carried out over two observing seasons suggest that the period found by Hintz et al. (1998) was no longer valid in early 1998, and that the period again changed during ...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2013
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/stt731