HT Cas - eclipsing dwarf nova during its superoutburst in 2010

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HT Cas.pdf (1.62 MB)

Publication date

2013

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Ciencias Integradas

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Center

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https://hdl.handle.net/10272/21751

DOI

10.48550/ARXIV.1312.5211

Abstract

We present results of a world-wide observing campaign of the eclips- ing dwarf nova - HT Cas during its superoutburst in November 2010. Using collected data we were able to conduct analysis of the light curves and we calculated O − C diagrams. The CCD photometric observations enabled us to derive the superhump period and with the timings of eclipses the orbital period was calculated. Based on superhump and orbital period estimations the period excess and mass ratio of the system were obtained.

Keywords

Stars; Individual; HT Cas - binaries; Close - novae, cataclysmic variables

Unesco Subjects

22 Física

Bibliographic citation

Bakowska, K., Olech, A., Rutkowski, A., Koff, R., de Miguel, E., & Otulakowska-Hypka, M. (2013). HT Cas - eclipsing dwarf nova during its superoutburst in 2010 (Version 1). arXiv. https://doi.org/10.48550/ARXIV.1312.5211

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