Add to ORKGI review the current knowledge of the long-term evolution of CVs and discuss the possible influence of a magnetic white dwarf on properties determining the observable orbital period distribution. (orig.)Available from TIB Hannover: RR 4697(871) / FIZ - Fachinformationszzentrum Karlsruhe / TIB - Technische InformationsbibliothekSIGLEDEGerman
accepted for publication in ApJThe population of non magnetic cataclysmic variables evolving under t...
Results of a CCD study of the variability of the unique magnetic cataclysmic variable V1432 Aql from...
Isolated magnetic white dwarfs have field strengths ranging from 10(3)G to 10(9) G, and constitute a...
We present system parameters for a small sample of short period, eclipsing CVs taken from the Sloan ...
A summary is presented of what is currently known about the surface temperatures of accreting white ...
Cataclysmic Variables (CV) are binary systems where a main-sequence star transfers mass onto a white...
The magnetic cataclysmic variables (MCVs) present a wealth of observational diagnostics for studying...
In this paper we review the current status of research on the observational and theoretical characte...
Cataclysmic Variables (CVs) are interacting binary systems comprised of a white dwarf (WD) and a sec...
We show that the recently discovered short period supersoft source in M31 is probably a progenitor o...
We report on the masses (MWD), effective temperatures (TeffTeff), andsecular mean accretion rates ...
I give an overview of the rich phenomenology of dwarf nova oscillations (DNOs) and Quasi-periodic Os...
The origin of magnetic fields in white dwarfs remains a fundamental unresolved problem in stellar as...
We present high-speed, three-colour photometry of seven short-period (P-orb <= 95 min) eclipsing cat...
International audienceA central hypothesis in the theory of cataclysmic variable (CV) evolution is t...
accepted for publication in ApJThe population of non magnetic cataclysmic variables evolving under t...
Results of a CCD study of the variability of the unique magnetic cataclysmic variable V1432 Aql from...
Isolated magnetic white dwarfs have field strengths ranging from 10(3)G to 10(9) G, and constitute a...
We present system parameters for a small sample of short period, eclipsing CVs taken from the Sloan ...
A summary is presented of what is currently known about the surface temperatures of accreting white ...
Cataclysmic Variables (CV) are binary systems where a main-sequence star transfers mass onto a white...
The magnetic cataclysmic variables (MCVs) present a wealth of observational diagnostics for studying...
In this paper we review the current status of research on the observational and theoretical characte...
Cataclysmic Variables (CVs) are interacting binary systems comprised of a white dwarf (WD) and a sec...
We show that the recently discovered short period supersoft source in M31 is probably a progenitor o...
We report on the masses (MWD), effective temperatures (TeffTeff), andsecular mean accretion rates ...
I give an overview of the rich phenomenology of dwarf nova oscillations (DNOs) and Quasi-periodic Os...
The origin of magnetic fields in white dwarfs remains a fundamental unresolved problem in stellar as...
We present high-speed, three-colour photometry of seven short-period (P-orb <= 95 min) eclipsing cat...
International audienceA central hypothesis in the theory of cataclysmic variable (CV) evolution is t...
accepted for publication in ApJThe population of non magnetic cataclysmic variables evolving under t...
Results of a CCD study of the variability of the unique magnetic cataclysmic variable V1432 Aql from...
Isolated magnetic white dwarfs have field strengths ranging from 10(3)G to 10(9) G, and constitute a...