The interest in studying multiple systems comes from the fact that they give a good number of constraints on their components. From the multiplicity we have constraints on mass and age. Moreover, if one or more components of the system show oscillating properties as the DG Leo triple system, additional constraints provided by seismology can be obtained once the modes are identified. In this work, we consider an equilibrium model of the DG Leo system constrained by its multiplicity properties, we attempt to check our new Time Depending Convection treatment on the modes identification of the DG Leo system
Context. Solar-like oscillations have been observed by Kepler and CoRoT in many solar-type stars, th...
Context. The late A and F-type γ Doradus (γ Dor) stars pulsate with high-order gravity modes (g-mode...
Context. A growing number of solar-like oscillations has been detected in red giant stars thanks to ...
peer reviewedWe apply for the first time the time-dependent convection (TDC) treatment of Gabriel an...
We apply the Time-Dependent Convection (TDC) treatment of Gabriel \cite{Gabriel1996} and Grigahcène ...
ABSTRACT Since the early days of helioseismology, adiabatic models have shown their limits for a pre...
International audienceWe apply for the first time the time-dependent convection (TDC) treatment of G...
Adiabatic modeling of solar-like oscillations cannot exceed a certain level of precision for fitting...
For delta Scuti stars, phase differences and amplitude ratios between the relative effective tempera...
Phase differences and amplitude ratios at different colour photometric bands are currently being use...
Stellar pulsations propagate through the star and carry with them information about the condition wi...
We apply the Levenberg-Marquardt minimization algorithm to seismic and classical observables of the ...
The asteroseismology of individual solar-like oscillators generally allows more precise inferences a...
The clear detection with CoRoT and Kepler of radial and non-radial solar-like oscillations in many r...
Context: The identification of pulsation modes in delta Scuti stars is mandatory for constraining th...
Context. Solar-like oscillations have been observed by Kepler and CoRoT in many solar-type stars, th...
Context. The late A and F-type γ Doradus (γ Dor) stars pulsate with high-order gravity modes (g-mode...
Context. A growing number of solar-like oscillations has been detected in red giant stars thanks to ...
peer reviewedWe apply for the first time the time-dependent convection (TDC) treatment of Gabriel an...
We apply the Time-Dependent Convection (TDC) treatment of Gabriel \cite{Gabriel1996} and Grigahcène ...
ABSTRACT Since the early days of helioseismology, adiabatic models have shown their limits for a pre...
International audienceWe apply for the first time the time-dependent convection (TDC) treatment of G...
Adiabatic modeling of solar-like oscillations cannot exceed a certain level of precision for fitting...
For delta Scuti stars, phase differences and amplitude ratios between the relative effective tempera...
Phase differences and amplitude ratios at different colour photometric bands are currently being use...
Stellar pulsations propagate through the star and carry with them information about the condition wi...
We apply the Levenberg-Marquardt minimization algorithm to seismic and classical observables of the ...
The asteroseismology of individual solar-like oscillators generally allows more precise inferences a...
The clear detection with CoRoT and Kepler of radial and non-radial solar-like oscillations in many r...
Context: The identification of pulsation modes in delta Scuti stars is mandatory for constraining th...
Context. Solar-like oscillations have been observed by Kepler and CoRoT in many solar-type stars, th...
Context. The late A and F-type γ Doradus (γ Dor) stars pulsate with high-order gravity modes (g-mode...
Context. A growing number of solar-like oscillations has been detected in red giant stars thanks to ...