In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 45, no. 2
S. Shugarov - N. Katysheva - N. Gladilina
Details:
Year, pages: 2015, 119 - 130
Keywords:
dwarf novae, photometry, suberoutburst, superhumps
Original source URL: http://www.astro.sk/caosp/Eedition/Abstracts/2015/Vol_45/No_2/pp119-130_abstract.html
About article:
Analysis of the photometric behavior of the WZ Sge-type object PR Herculis
during the 2011 outburst was carried out. The periods of "early"
(0.05424d) and "ordinary" (0.054990d) superhumps were
determined. The value of Pdot=4.7 10-5,
showing the rate of change of the period of "ordinary" superhumps
during the superoutburst, was found.
How to cite:
ISO 690:
Shugarov, S., Katysheva, N., Gladilina, N. 2015. PR Her — a WZ Sge-type cataclysmic variable. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 45, no.2, pp. 119-130. 1335-1842.
APA:
Shugarov, S., Katysheva, N., Gladilina, N. (2015). PR Her — a WZ Sge-type cataclysmic variable. Contributions of the Astronomical Observatory Skalnaté Pleso, 45(2), 119-130. 1335-1842.