PR Her — a WZ Sge-type cataclysmic variable

In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 45, no. 2

S. Shugarov - N. Katysheva - N. Gladilina

Detaily:

Rok, strany: 2015, 119 - 130

Kľúčové slová:

dwarf novae, photometry, suberoutburst, superhumps

URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2015/Vol_45/No_2/pp119-130_abstract.html

Full text

O článku:

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 P_dot=4.7 10^-5, showing the rate of change of the period of "ordinary" superhumps during the superoutburst, was found.

Ako citovať:

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.