These files contain the inlist and net file needed to reproduce the A0 model in the associated paper
Diffusion of elements in the atmosphere of a star can drastically affect its surface composition, so...
Context. The benchmark open cluster M 67 is known to have solar metallicity and an age similar to th...
Abstract. The nuclides 1,2H, 3,4He, 7Li, 7Be, 8B, 12,13C, 13-15N, 14-18O, 17-19F, 18-22Ne, 22Mg, and...
Context. The stellar evolution code Modules for Experiments in Stellar Astrophysics (MESA) is public...
This book gives an overview of atomic diffusion, a fundamental physical process, as applied to all t...
International audienceStellar physics and evolution calculations enable a broad range of research in...
MESA inlist files that were used to calculate metal-free evolutionary models for the publication Lar...
Atomic diffusion in stars is efficient in changing the distribution of elements slowly but strongly ...
We update the capabilities of the software instrument Modules for Experiments in Stellar Astrophysic...
Input files (inlists) used to compute MESA binary models to paper "Partial-envelope stripping and nu...
Stellar models including atomic diffusion processes (gravitational settling, radiative accelerations...
We present recent work undertaken by the Evolution and Seismic Tools Activity (ESTA) team of the CoR...
Aims. Atomic diffusion, including the effect of radiative accelerations on individual elements, lead...
We update the capabilities of the open-knowledge software instrument Modules for Experiments in Stel...
Atomic diffusion in stars may affect element distributions in layers where mixing motions are weak e...
Diffusion of elements in the atmosphere of a star can drastically affect its surface composition, so...
Context. The benchmark open cluster M 67 is known to have solar metallicity and an age similar to th...
Abstract. The nuclides 1,2H, 3,4He, 7Li, 7Be, 8B, 12,13C, 13-15N, 14-18O, 17-19F, 18-22Ne, 22Mg, and...
Context. The stellar evolution code Modules for Experiments in Stellar Astrophysics (MESA) is public...
This book gives an overview of atomic diffusion, a fundamental physical process, as applied to all t...
International audienceStellar physics and evolution calculations enable a broad range of research in...
MESA inlist files that were used to calculate metal-free evolutionary models for the publication Lar...
Atomic diffusion in stars is efficient in changing the distribution of elements slowly but strongly ...
We update the capabilities of the software instrument Modules for Experiments in Stellar Astrophysic...
Input files (inlists) used to compute MESA binary models to paper "Partial-envelope stripping and nu...
Stellar models including atomic diffusion processes (gravitational settling, radiative accelerations...
We present recent work undertaken by the Evolution and Seismic Tools Activity (ESTA) team of the CoR...
Aims. Atomic diffusion, including the effect of radiative accelerations on individual elements, lead...
We update the capabilities of the open-knowledge software instrument Modules for Experiments in Stel...
Atomic diffusion in stars may affect element distributions in layers where mixing motions are weak e...
Diffusion of elements in the atmosphere of a star can drastically affect its surface composition, so...
Context. The benchmark open cluster M 67 is known to have solar metallicity and an age similar to th...
Abstract. The nuclides 1,2H, 3,4He, 7Li, 7Be, 8B, 12,13C, 13-15N, 14-18O, 17-19F, 18-22Ne, 22Mg, and...
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