I review, from an observational perspective, the interactions of accretion discs with magnetic fields in cataclysmic variable stars. I start with systems where the accretion flows via a stream, and discuss the circumstances in which the stream forms into an accretion disc, pointing to stars which are close to this transition. I then turn to disc-fed systems and discuss what we know about how material threads on to field lines, as deduced from the pattern of accretion footprints on the white dwarf. I discuss whether distortions of the field lines are related to accretion torques and the changing spin periods of the white dwarfs. I also review the effect on the disc-magnetosphere interaction of disc-instability outbursts. Lastly, I discuss th...
International audienceContext. The disc instability model (DIM) has been very successful in explaini...
International audienceContext. The disc instability model (DIM) has been very successful in explaini...
The dwarf nova oscillations observed in cataclysmic variable (CV) stars are interpreted in the conte...
I review, from an observational perspective, the interactions of accretion discs with magnetic field...
The magnetic cataclysmic variables (MCVs) present a wealth of observational diagnostics for studying...
Abstract. The Magnetic Cataclysmic Variables (MCVs) are close interacting binaries where mass is tra...
This thesis explores aspects of the theory of accretion discs in two astrophysical environments; aro...
secondary. In non-magnetic cataclysmic variables (CVs) a white dwarf accretes matter from a main-seq...
Accretion discs are commonplace around magnetic stars. They can be found in newly formed stars and ...
The Magnetic Cataclysmic Variables (MCVs) are close interacting binaries where mass is transferred f...
The Magnetic Cataclysmic Variables (MCVs) are close interacting binaries where mass is transferred f...
Many observations indicate that fast rotating late type stars show magnetic activity. We therefore a...
The magnetic cataclysmic variables (MCVs) present a wealth of observational diagnostics for studying...
Disk accretion onto magnetic stars occurs in a variety of systems, including accreting neutron stars...
This thesis discusses the interaction of stellar magnetic fields with circumstellar material in a va...
International audienceContext. The disc instability model (DIM) has been very successful in explaini...
International audienceContext. The disc instability model (DIM) has been very successful in explaini...
The dwarf nova oscillations observed in cataclysmic variable (CV) stars are interpreted in the conte...
I review, from an observational perspective, the interactions of accretion discs with magnetic field...
The magnetic cataclysmic variables (MCVs) present a wealth of observational diagnostics for studying...
Abstract. The Magnetic Cataclysmic Variables (MCVs) are close interacting binaries where mass is tra...
This thesis explores aspects of the theory of accretion discs in two astrophysical environments; aro...
secondary. In non-magnetic cataclysmic variables (CVs) a white dwarf accretes matter from a main-seq...
Accretion discs are commonplace around magnetic stars. They can be found in newly formed stars and ...
The Magnetic Cataclysmic Variables (MCVs) are close interacting binaries where mass is transferred f...
The Magnetic Cataclysmic Variables (MCVs) are close interacting binaries where mass is transferred f...
Many observations indicate that fast rotating late type stars show magnetic activity. We therefore a...
The magnetic cataclysmic variables (MCVs) present a wealth of observational diagnostics for studying...
Disk accretion onto magnetic stars occurs in a variety of systems, including accreting neutron stars...
This thesis discusses the interaction of stellar magnetic fields with circumstellar material in a va...
International audienceContext. The disc instability model (DIM) has been very successful in explaini...
International audienceContext. The disc instability model (DIM) has been very successful in explaini...
The dwarf nova oscillations observed in cataclysmic variable (CV) stars are interpreted in the conte...