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- W2068841247 abstract "Recent work on Ultra Long Period Cepheids (ULPCs) has suggested their usefulness as a distance indicator, but has not commented on their relationship as compared with other types of variable stars. In this work, we use Fourier analysis to quantify the structure of ULPC light curves and compare them to Classical Cepheids and Mira variables. Our preliminary results suggest that the low order Fourier parameters (R <sub xmlns:mml=http://www.w3.org/1998/Math/MathML xmlns:xlink=http://www.w3.org/1999/xlink>k1</sub> and φ <sub xmlns:mml=http://www.w3.org/1998/Math/MathML xmlns:xlink=http://www.w3.org/1999/xlink>k1</sub> ) of ULPCs show a continuous trend defined by Classical Cepheids after the resonance around 10 days. However their Fourier parameters also overlapped with those from Miras, which make the classification of long period variable stars difficult based on the light curves information alone." @default.
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- W2068841247 date "2013-07-01" @default.
- W2068841247 modified "2023-09-27" @default.
- W2068841247 title "Preliminary analysis of ULPC light curves using fourier decomposition technique" @default.
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- W2068841247 doi "https://doi.org/10.1109/iconspace.2013.6599423" @default.
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