Add to ORKGA detailed understanding of the secondary stars in cataclysmic variables (CVs) and other mass-transferring binaries is of vital importance if we are to fully understand the behavior and evolution of such systems. Magnetic activity, for example, plays an important role in the angular momentum evolution of the binary and has also been linked to the orbital period, mean brightness and mean outburst duration of CVs.EThOS - Electronic Theses Online ServiceGBUnited Kingdo
We present spectroscopy of four cataclysmic variables. Using radial velocity measurements, we find o...
This thesis explores the cataclysmic variables (CVs) found by the Palomar-Green (PG) survey. This is...
Cataclysmic variables are binary stars in which a relatively normal star is transferring mass to its...
The secondary, Roche-lobe filling stars in cataclysmic variables (CVs) are key to our understanding ...
Cataclysmic variable stars are semi-detached binary systems consisting of a white dwarf primary star...
We present a set of Roche tomography reconstructions of the secondary stars in the cataclysmic varia...
We present a Roche tomography reconstruction of the secondary star in the cataclysmic variable AE Aq...
Cataclysmic variables are binary stars in which a relatively normal star is transferring mass to its...
SIGLEAvailable from British Library Document Supply Centre- DSC:DXN060478 / BLDSC - British Library ...
We present Roche tomograms of the secondary star in the dwarf nova system RU Pegasi derived from blu...
We present Roche tomograms of the G5–G8 IV/V secondary star in the long-period cataclysmic variable ...
Cataclysmic variable stars (CVs) are interacting binary systems. One of the stars (referred to as th...
International audienceWe present the results of our spectroscopic study of the dwarf nova SS Cyg, us...
The commissioning year of the Sloan Digital Sky Survey (SDSS) has demonstrated that many cataclysmic...
We give a global analysis of mass transfer variations in CVs. We show that limit cycles driven by va...
We present spectroscopy of four cataclysmic variables. Using radial velocity measurements, we find o...
This thesis explores the cataclysmic variables (CVs) found by the Palomar-Green (PG) survey. This is...
Cataclysmic variables are binary stars in which a relatively normal star is transferring mass to its...
The secondary, Roche-lobe filling stars in cataclysmic variables (CVs) are key to our understanding ...
Cataclysmic variable stars are semi-detached binary systems consisting of a white dwarf primary star...
We present a set of Roche tomography reconstructions of the secondary stars in the cataclysmic varia...
We present a Roche tomography reconstruction of the secondary star in the cataclysmic variable AE Aq...
Cataclysmic variables are binary stars in which a relatively normal star is transferring mass to its...
SIGLEAvailable from British Library Document Supply Centre- DSC:DXN060478 / BLDSC - British Library ...
We present Roche tomograms of the secondary star in the dwarf nova system RU Pegasi derived from blu...
We present Roche tomograms of the G5–G8 IV/V secondary star in the long-period cataclysmic variable ...
Cataclysmic variable stars (CVs) are interacting binary systems. One of the stars (referred to as th...
International audienceWe present the results of our spectroscopic study of the dwarf nova SS Cyg, us...
The commissioning year of the Sloan Digital Sky Survey (SDSS) has demonstrated that many cataclysmic...
We give a global analysis of mass transfer variations in CVs. We show that limit cycles driven by va...
We present spectroscopy of four cataclysmic variables. Using radial velocity measurements, we find o...
This thesis explores the cataclysmic variables (CVs) found by the Palomar-Green (PG) survey. This is...
Cataclysmic variables are binary stars in which a relatively normal star is transferring mass to its...