Add to ORKGWe show that the recently discovered short period supersoft source in M31 is probably a progenitor of a magnetic cataclysmic variable (CV). The white dwarf spins asynchronously because of the current high accretion rate. However its fieldstrength is typical of an AM Herculis system, which is what it will ultimately become. We discuss the relevance of this system to CV evolution, and its relation to some particular CVs with special characteristics
We present high-speed, three-colour photometry of seven short-period (P-orb <= 95 min) eclipsing cat...
WOS: 000400504900015We present a binary evolution study of cataclysmic variables (CVs) and related s...
White dwarfs with surface magnetic fields in excess of 1 MG are found as isolated single stars and r...
We show that the recently discovered short period supersoft source in M31 is probably a progenitor o...
I review the current knowledge of the long-term evolution of CVs and discuss the possible influence ...
AM Her variables - synchronized magnetic cataclysmic variables (CVs) - exhibit a different period di...
We have used a model of magnetic accretion to investigate the accretion flows of magnetic cataclysmi...
Current treatments of accretion flows in magnetic cataclysmic variables (CVs) imply that the criteri...
We present system parameters for a small sample of short period, eclipsing CVs taken from the Sloan ...
We present an attempt to reconstruct the complete evolutionary path followed by cataclysmic variable...
International audienceContext. Observations of cataclysmic variables in globular clusters appear to ...
I give an overview of the rich phenomenology of dwarf nova oscillations (DNOs) and Quasi-periodic Os...
Cataclysmic Variables (CV) are binary systems where a main-sequence star transfers mass onto a white...
We present the results of simulations that explore the variety of accretion flows possible in magnet...
SDSS J090221.35+381941.9 is an Cataclysmic Variable AM CVn system that has three most likely evoluti...
We present high-speed, three-colour photometry of seven short-period (P-orb <= 95 min) eclipsing cat...
WOS: 000400504900015We present a binary evolution study of cataclysmic variables (CVs) and related s...
White dwarfs with surface magnetic fields in excess of 1 MG are found as isolated single stars and r...
We show that the recently discovered short period supersoft source in M31 is probably a progenitor o...
I review the current knowledge of the long-term evolution of CVs and discuss the possible influence ...
AM Her variables - synchronized magnetic cataclysmic variables (CVs) - exhibit a different period di...
We have used a model of magnetic accretion to investigate the accretion flows of magnetic cataclysmi...
Current treatments of accretion flows in magnetic cataclysmic variables (CVs) imply that the criteri...
We present system parameters for a small sample of short period, eclipsing CVs taken from the Sloan ...
We present an attempt to reconstruct the complete evolutionary path followed by cataclysmic variable...
International audienceContext. Observations of cataclysmic variables in globular clusters appear to ...
I give an overview of the rich phenomenology of dwarf nova oscillations (DNOs) and Quasi-periodic Os...
Cataclysmic Variables (CV) are binary systems where a main-sequence star transfers mass onto a white...
We present the results of simulations that explore the variety of accretion flows possible in magnet...
SDSS J090221.35+381941.9 is an Cataclysmic Variable AM CVn system that has three most likely evoluti...
We present high-speed, three-colour photometry of seven short-period (P-orb <= 95 min) eclipsing cat...
WOS: 000400504900015We present a binary evolution study of cataclysmic variables (CVs) and related s...
White dwarfs with surface magnetic fields in excess of 1 MG are found as isolated single stars and r...