The approximation known as Frozen Convection has been widely used in the context of stellar oscillations due to the lack of a Time Dependent Convection theory. This approximation supposes to neglect the interaction between convection and oscillations and there are different ways to do it. The choice can affect theoretical predictions concerning the non-adiabatic treatment of the stellar oscillations. In fact, fictitious excitation or damping of the pulsation modes can be produced depending on the approximation used
International audienceWe apply for the first time time-dependent convection (TDC) models to the stud...
International audienceWe apply for the first time time-dependent convection (TDC) models to the stud...
Adiabatic modeling of solar-like oscillations cannot exceed a certain level of precision for fitting...
The approximation known as Frozen Convection has been widely used in the context of stellar oscillat...
This article reviews our current understanding of modelling convection dynamics in stars. Several se...
This article reviews our current understanding of modelling convection dynamics in stars. Several se...
The coupling between convection and non-radial oscillations is discussed. The limitation of the theo...
Context. In Cepheids close to the red edge of the classical instability strip, a coupling occurs bet...
peer reviewedThe problem of the interaction between convection and pulsations is considered. A preci...
peer reviewedSince the early days of helioseismology, adiabatic models have shown their limits for a...
peer reviewedSince the early days of helioseismology, adiabatic models have shown their limits for a...
ABSTRACT Since the early days of helioseismology, adiabatic models have shown their limits for a pre...
We apply here the Time Dependent Convection (TDC) treatment presented in our earlier paper in this s...
We present in details a time-dependent convection treatment in the frame of the Mixing-Length Theory...
We present in details a time-dependent convection treatment in the frame of the Mixing-Length Theory...
International audienceWe apply for the first time time-dependent convection (TDC) models to the stud...
International audienceWe apply for the first time time-dependent convection (TDC) models to the stud...
Adiabatic modeling of solar-like oscillations cannot exceed a certain level of precision for fitting...
The approximation known as Frozen Convection has been widely used in the context of stellar oscillat...
This article reviews our current understanding of modelling convection dynamics in stars. Several se...
This article reviews our current understanding of modelling convection dynamics in stars. Several se...
The coupling between convection and non-radial oscillations is discussed. The limitation of the theo...
Context. In Cepheids close to the red edge of the classical instability strip, a coupling occurs bet...
peer reviewedThe problem of the interaction between convection and pulsations is considered. A preci...
peer reviewedSince the early days of helioseismology, adiabatic models have shown their limits for a...
peer reviewedSince the early days of helioseismology, adiabatic models have shown their limits for a...
ABSTRACT Since the early days of helioseismology, adiabatic models have shown their limits for a pre...
We apply here the Time Dependent Convection (TDC) treatment presented in our earlier paper in this s...
We present in details a time-dependent convection treatment in the frame of the Mixing-Length Theory...
We present in details a time-dependent convection treatment in the frame of the Mixing-Length Theory...
International audienceWe apply for the first time time-dependent convection (TDC) models to the stud...
International audienceWe apply for the first time time-dependent convection (TDC) models to the stud...
Adiabatic modeling of solar-like oscillations cannot exceed a certain level of precision for fitting...