CAOSP abstracts, Volume: 45, No.: 2, year: 2015

Abstract: 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.

Full text version of this article in PostScript (600dpi) format compressed by gzip; or in PDF.

Back to:
CAOSP Vol. 45 No. 2 index
CAOSP archive main index
CAOSP main page
Astronomical Institute home page
Valid XHTML 1.0! Valid CSS!

Last update: January 13, 2016