CAOSP abstracts, Volume: 43, No.: 3, year: 2014

Abstract: Quasi-periodic oscillations (QPOs) are rapid variations in brightness of cataclysmic variables (CVs). They are most probably caused by a magnetically excited wave in the accretion disc. No spectroscopic observations of these phenomena have been published yet. We will attempt to carry out both photometric and spectrophotometric time-resolved observations of a QPO. Observations will be carried out with two telescopes at the same time - one of the telescopes is working with an objective prism, handling spectroscopic data. The second one is used for photometry.

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

Back to:
CAOSP Vol. 43 No. 3 index
CAOSP archive main index
CAOSP main page
Astronomical Institute home page
Valid XHTML 1.0! Valid CSS!

Last update: April 17, 2014