We present a first application of Whosglad method to the components A and B of the 16 Cygni system. The method was developed to provide a comprehensive analysis of stellar oscillation spectra. It defines new seismic indicators which are as uncorrelated and precise as possible and hold detailed information about stellar interiors. Such indicators, as illustrated in the present paper, may be used to generate stellar models via forward seismic modeling. Finally, seismic constraints retrieved by the method provide realistic stellar parameters
International audienceWe present grids of stellar models and their associated oscillation frequencie...
The Stellar Seismic Indices database (hereafter SSI) has been developed within the SPACEInn project ...
International audienceContext. Seismic parameters such as the large Delta0 and small delta02 frequen...
We present a first application of Whosglad method to the components A and B of the 16 Cygni system. ...
International audienceContext. Being part of the brightest solar-like stars, and close solar analogu...
Aims: We develop a method that provides a comprehensive analysis of the oscillation spectra of solar...
Context. Being part of the brightest solar-like stars, and close solar analogues, the 16 Cygni syste...
International audienceContext. The advent of space-based photometry observations provided high-quali...
peer reviewedContext: Being part of the brightest solar-like stars, and close solar analogues, the 1...
We present a method for measuring internal stellar structure based on asteroseismology that we call ...
International audienceContext. Constraining additional mixing processes and chemical composition is ...
International audienceIndependent of stellar modelling, global seismic parameters of red giants prov...
High precision and long-lasting Kepler data enabled us to estimate stellar properties with asterosei...
International audienceWe present grids of stellar models and their associated oscillation frequencie...
The Stellar Seismic Indices database (hereafter SSI) has been developed within the SPACEInn project ...
International audienceContext. Seismic parameters such as the large Delta0 and small delta02 frequen...
We present a first application of Whosglad method to the components A and B of the 16 Cygni system. ...
International audienceContext. Being part of the brightest solar-like stars, and close solar analogu...
Aims: We develop a method that provides a comprehensive analysis of the oscillation spectra of solar...
Context. Being part of the brightest solar-like stars, and close solar analogues, the 16 Cygni syste...
International audienceContext. The advent of space-based photometry observations provided high-quali...
peer reviewedContext: Being part of the brightest solar-like stars, and close solar analogues, the 1...
We present a method for measuring internal stellar structure based on asteroseismology that we call ...
International audienceContext. Constraining additional mixing processes and chemical composition is ...
International audienceIndependent of stellar modelling, global seismic parameters of red giants prov...
High precision and long-lasting Kepler data enabled us to estimate stellar properties with asterosei...
International audienceWe present grids of stellar models and their associated oscillation frequencie...
The Stellar Seismic Indices database (hereafter SSI) has been developed within the SPACEInn project ...
International audienceContext. Seismic parameters such as the large Delta0 and small delta02 frequen...