Photometric Study of a Nova-Like Cataclysmic Variable Star NSV 25181

Details Photometric Study of a Nova-Like Cataclysmic Variable Star NSV 25181 Photometric Study of a Nova-Like Cataclysmic Variable Star NSV 25181

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ibvs.5956....1z&link_type=abstract

Information Bulletin on Variable Stars, 5956, 1.

Physics

Stars: Cataclysmic Variables

Scientific paper

We confirm variability of NSV 25181 on the base of our CCD observations
and find three kinds of variations: slow night-to-night brightness
changes, strong flickering and periodic variability (possibly non-radial
pulsations of the white dwarf).

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