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- W2261089510 abstract "In this work we present the results of light curve analysis for two cataclysmic variables detected recently in the SDSS project: SDSS J090350.73+330036.1 and J150240.98+333423.9. Photometric observations of the first were obtained during a superoutburst in May 2010. Our observations clearly indicate the presence of superhumps in the light curves, suggesting SDSS J090350.73+330036.1 is an SU UMa dwarf nova. We determined the period of the superhumps. We also carried out fitting using a spiral-arm model in order to determine parameters of the accretion disk, hot line, and other components of this system. Photometric observations of the second, J150240.98+333423.9, were obtained during the post-maximum decline, during April-June 2012. Photometric variability of this system has been studied in an inactive state. We obtained its parameters via a combined model fitted to the observed light curves by x 2 minimization." @default.
- W2261089510 created "2016-06-24" @default.
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- W2261089510 date "2015-09-30" @default.
- W2261089510 modified "2023-09-27" @default.
- W2261089510 title "STUDY OF SUPERHUMPS IN THE RECENTLY DISCOVERED SU UMA DWARF NOVAE" @default.
- W2261089510 cites W174186847 @default.
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- W2261089510 doi "https://doi.org/10.5303/pkas.2015.30.2.241" @default.
- W2261089510 hasPublicationYear "2015" @default.
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