Add to ORKGInfluence of non-adiabatic temperature variations on line prole variations of slowly rotating Cep stars and SPBs I. Non-adiabatic eigenfunctions in the atmosphere of a pulsating sta
. We present a computing code for modelling energy flux distributions, photometric indices and spec...
A new general method for the computation of nonradial nonadiabatic oscillations of a given stellar m...
He i 6678 in the periodic Be star 28 CMa. A simple zeroth-order approximation to the eigenfunctions ...
peer reviewedIn this study, we compute theoretical line profiles of a non-radially pulsating star, t...
We investigate to what extent non-adiabatic temperature variations at the surface of slowly rotati...
We investigate to what extent non-adiabatic temperature variations at the surface of slowly rotating...
International audienceOne of the greatest challenges in interpreting the pulsations of rapidly rotat...
Abstract. Phase differences and amplitude ratios at different colour photometric bands are currently...
We present a useful formulation of the surface-velocity field of a rotating, adiabatically pulsating...
Eddington, Schwarzschild, Woltjer and others have discussed the Non-adiabatic Pulsations of a Star i...
Title Line-profile variations of non-radial adiabetic pulsations of rotating stars II. The diagnosti...
For delta Scuti stars, phase differences and amplitude ratios between the relative effective tempera...
This paper explores the effect of rotation on the kappa-mechanism instability of slowly pulsating B ...
Title Line-profile variations due to adiabetic non-radial pulsations in rotating stars. IV The effec...
Taking into account non-adiabatic effects in stellar pulsation calculations is important because it ...
. We present a computing code for modelling energy flux distributions, photometric indices and spec...
A new general method for the computation of nonradial nonadiabatic oscillations of a given stellar m...
He i 6678 in the periodic Be star 28 CMa. A simple zeroth-order approximation to the eigenfunctions ...
peer reviewedIn this study, we compute theoretical line profiles of a non-radially pulsating star, t...
We investigate to what extent non-adiabatic temperature variations at the surface of slowly rotati...
We investigate to what extent non-adiabatic temperature variations at the surface of slowly rotating...
International audienceOne of the greatest challenges in interpreting the pulsations of rapidly rotat...
Abstract. Phase differences and amplitude ratios at different colour photometric bands are currently...
We present a useful formulation of the surface-velocity field of a rotating, adiabatically pulsating...
Eddington, Schwarzschild, Woltjer and others have discussed the Non-adiabatic Pulsations of a Star i...
Title Line-profile variations of non-radial adiabetic pulsations of rotating stars II. The diagnosti...
For delta Scuti stars, phase differences and amplitude ratios between the relative effective tempera...
This paper explores the effect of rotation on the kappa-mechanism instability of slowly pulsating B ...
Title Line-profile variations due to adiabetic non-radial pulsations in rotating stars. IV The effec...
Taking into account non-adiabatic effects in stellar pulsation calculations is important because it ...
. We present a computing code for modelling energy flux distributions, photometric indices and spec...
A new general method for the computation of nonradial nonadiabatic oscillations of a given stellar m...
He i 6678 in the periodic Be star 28 CMa. A simple zeroth-order approximation to the eigenfunctions ...