Add to ORKGIncludes bibliographical references.The roAp stars are high overtone pulsators characterised by stro...
In 1995 we initiated a Northern Hemisphere survey for rapidly oscillating Ap stars. This paper prese...
We have carried out the first survey of the pulsational line profile variability in rapidly oscillat...
I review recent theoretical work on rapidly oscillating Ap stars and discuss key aspects of the phys...
Rapidly oscillating Ap stars constitute a unique class of pulsators with which to study non-radial o...
Abstract. This paper reviews some of the important advances made over the last decade concerning the...
I review recent results of the observations of magnetoacoustic p-mode oscillations in roAp stars wit...
The oblique pulsator model accounts for most of the pulsation properties of the rapidly oscillating...
The oblique pulsator model accounts for most of the pulsation properties of the rapidly oscillating...
Chemically peculiar stars are stage to a wide variety of physical phenomena, including diffusion, co...
Chemically peculiar stars are stage to a wide variety of physical phenomena, including diffusion, co...
Context. The dipole modes are the most common geometry of oscillations in roAp stars inferred from...
The rapidly oscillating Ap (roAp) stars provide a unique opportunity to observe and test processes ...
The rapidly oscillating Ap (roAp) stars are a sub-group of the chemically peculiar stars of class 2 ...
In the presence of a magnetic field, stellar spectral lines may appear systematically broader in one...
Includes bibliographical references.The roAp stars are high overtone pulsators characterised by stro...
In 1995 we initiated a Northern Hemisphere survey for rapidly oscillating Ap stars. This paper prese...
We have carried out the first survey of the pulsational line profile variability in rapidly oscillat...
I review recent theoretical work on rapidly oscillating Ap stars and discuss key aspects of the phys...
Rapidly oscillating Ap stars constitute a unique class of pulsators with which to study non-radial o...
Abstract. This paper reviews some of the important advances made over the last decade concerning the...
I review recent results of the observations of magnetoacoustic p-mode oscillations in roAp stars wit...
The oblique pulsator model accounts for most of the pulsation properties of the rapidly oscillating...
The oblique pulsator model accounts for most of the pulsation properties of the rapidly oscillating...
Chemically peculiar stars are stage to a wide variety of physical phenomena, including diffusion, co...
Chemically peculiar stars are stage to a wide variety of physical phenomena, including diffusion, co...
Context. The dipole modes are the most common geometry of oscillations in roAp stars inferred from...
The rapidly oscillating Ap (roAp) stars provide a unique opportunity to observe and test processes ...
The rapidly oscillating Ap (roAp) stars are a sub-group of the chemically peculiar stars of class 2 ...
In the presence of a magnetic field, stellar spectral lines may appear systematically broader in one...
Includes bibliographical references.The roAp stars are high overtone pulsators characterised by stro...
In 1995 we initiated a Northern Hemisphere survey for rapidly oscillating Ap stars. This paper prese...
We have carried out the first survey of the pulsational line profile variability in rapidly oscillat...