CLÉS is an evolution code recently developed to produce stellar models meeting the specific requirements of studies in asteroseismology. It offers the users a lot of choices in the input physics they want in their models and its versatility allows them to tailor the code to their needs and implement easily new features. We describe the features implemented in the current version of the code and the techniques used to solve the equations of stellar structure and evolution. A brief account is given of the use of the program and of a solar calibration realized with it
We present and discuss evolutionary synthesis models for massive stellar populations generated with ...
Grid of evolutionary tracks with CLES (Scuflaire et al. 08). Version 19.2 (August 2019). Initial ch...
The aim of this thesis is to study stellar evolution and asteroseimology of red-giant stars mainly f...
International audienceCLÉS is an evolution code recently developed to produce stellar models meeting...
Abstract In this paper we present a grid of stellar evolution models, computed with an up-to-date p...
This paper presents the Geneva stellar evolution code with special emphasis on the modeling of solar...
We present the COLIBRI code for computing the evolution of stars along the thermally pulsing asympto...
Stellar physics groups different fields which come from hydrodynamic modelisation to asteroseismolog...
The Liège Oscillation code can be used as a stand-alone program or as a library of subroutines that ...
Aims: We develop a method that provides a comprehensive analysis of the oscillation spectra of solar...
The code CESAM is a consistent set of programs and routines which performs calculations of 1D quasi-...
This contribution is not about the quality of the agreement between stellar models computed by CESAM...
PARSEC (PAdova-TRieste Stellar Evolution Code) is the updated version of the the stellar evolution c...
This contribution is meant as a very brief introduction to the principal concepts of stellar physics...
We summarize the main physical assumptions and numerical procedures adopted by the FRANEC code to co...
We present and discuss evolutionary synthesis models for massive stellar populations generated with ...
Grid of evolutionary tracks with CLES (Scuflaire et al. 08). Version 19.2 (August 2019). Initial ch...
The aim of this thesis is to study stellar evolution and asteroseimology of red-giant stars mainly f...
International audienceCLÉS is an evolution code recently developed to produce stellar models meeting...
Abstract In this paper we present a grid of stellar evolution models, computed with an up-to-date p...
This paper presents the Geneva stellar evolution code with special emphasis on the modeling of solar...
We present the COLIBRI code for computing the evolution of stars along the thermally pulsing asympto...
Stellar physics groups different fields which come from hydrodynamic modelisation to asteroseismolog...
The Liège Oscillation code can be used as a stand-alone program or as a library of subroutines that ...
Aims: We develop a method that provides a comprehensive analysis of the oscillation spectra of solar...
The code CESAM is a consistent set of programs and routines which performs calculations of 1D quasi-...
This contribution is not about the quality of the agreement between stellar models computed by CESAM...
PARSEC (PAdova-TRieste Stellar Evolution Code) is the updated version of the the stellar evolution c...
This contribution is meant as a very brief introduction to the principal concepts of stellar physics...
We summarize the main physical assumptions and numerical procedures adopted by the FRANEC code to co...
We present and discuss evolutionary synthesis models for massive stellar populations generated with ...
Grid of evolutionary tracks with CLES (Scuflaire et al. 08). Version 19.2 (August 2019). Initial ch...
The aim of this thesis is to study stellar evolution and asteroseimology of red-giant stars mainly f...