In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 43, no. 3
K. Bąkowska - A. Olech - A. Rutkowski - R. Koff - E. De Miguel - M. Otulakowska-Hypka
Details:
Year, pages: 2014, 325 - 329
Keywords:
Stars: individual: HT Cas, binaries: close, novae, cataclysmic variables
Original source URL: http://www.astro.sk/caosp/Eedition/Abstracts/2014/Vol_43/No_3/pp325-329_abstract.html
About article:
We present results of a world-wide observing campaign of the eclipsing dwarf nova HT Cas during its superoutburst in November 2010. Using collected data we were able to conduct an 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.
How to cite:
ISO 690:
Bąkowska, K., Olech, A., Rutkowski, A., Koff, R., De Miguel, E., Otulakowska-Hypka, M. 2014. HT Cas - eclipsing dwarf nova during its superoutburst in 2010. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 43, no.3, pp. 325-329. 1335-1842.
APA:
Bąkowska, K., Olech, A., Rutkowski, A., Koff, R., De Miguel, E., Otulakowska-Hypka, M. (2014). HT Cas - eclipsing dwarf nova during its superoutburst in 2010. Contributions of the Astronomical Observatory Skalnaté Pleso, 43(3), 325-329. 1335-1842.