Influence of the velocity gradient on the line formation in discs of cataclysmic variables variables (CVs) is usually neglected; however, the geometry of the system and the value of Keplerian
Investigation of the new cataclysmic variable 1RXS J180834.7+101041 cataclysmic
variable star 1RXS J180834. 7+101041. Its spectrum exhibits double-peaked hydrogen and helium
THE CONCEPT "STAR" IN THE RUSSIAN AND CHINESE LANGUAGE PICTURE OF THE WORLD. The conceptual meanings of the cosmonym "
star" for the two linguistic cultures are
peculiar .
HBHA 4705-03: A new cataclysmic variableResults of photometric and spectroscopic studies for the new eclipsing cataclysmic
variable star Aperiodic optical variability of intermediate polars-cataclysmic variables with truncated accretion disksRevnivtsev M.,
Burenin R.,
Bikmaev I.,
Kniazev A.,
Buckley D.,
Pretorius M.,
Khamitov I.,
Ak T.,
Eker Z.,
Melnikov S.,
Crawford S.,
Pavlinsky M. We study the power spectra of the
variability of seven intermediate polars containing magnetized
A search for periodic and quasi-periodic photometric behavior in the cataclysmic variable TT arietisAndronov I.,
Arai K.,
Chinarova L.,
Dorokhov N.,
Dorokhova T.,
Dumitrescu A.,
Nogami D.,
Kolesnikov S.,
Lepardo A.,
Mason P.,
Matsumoto K.,
Oprescu G.,
Pajdosz G.,
Passuelo R.,
Patkos L.,
Senio D.,
Sostero G.,
Suleimanov V.,
Tremko J.,
Zhukov G.,
Zola S. out to study optical
variability on timescales from minutes to weeks. The best-fit primary photometric
Dwarf nova EZ Lyncis second visit to instability strip of observations, but with
variable amplitudes and
variable drifts of frequencies by 2%-6% on a time scale of ∼5
MLS120126:042313+212951—A New Eclipsing Cataclysmic Variable in the Period Gap cataclysmic
variable MLS120126:042313+212951. We have found the system’s orbital period P=0.1034329 day