Contains fulltext : 132559.pdf (preprint version ) (Open Access
The general problem of pattern formation in biological development is described. One possible type ...
This book gives an overview of atomic diffusion, a fundamental physical process, as applied to all t...
International audienceStellar evolution models of a 0.8 Msolar star (Y=0.2352, Z=0.0001, ?=0.3) have...
We have computed a new grid of evolutionary subdwarf B star (sdB) models from the start of central H...
Context. The pulsation frequencies of early B-type stars cannot be reproduced using stellar models w...
We reexamine the theoretical instability domain of pulsating DB white dwarfs (DBV or V777 Her variab...
We present a new set of nonlinear, convective radial pulsation models for main-sequence stars comput...
This is an electronic version of an article published in The Astrophysical Journal Supplement Series...
Aims. Atomic diffusion, including the effect of radiative accelerations on individual elements, lead...
The evolution of a monoatomic layer, deposited on a substrate, is described by a dynamical model of ...
Context. The physical mechanism leading to the formation of the blue loop in the Hertzsprung–Russell...
We present new grids of evolutionary models for the so-called “Anomalous” Cepheids (ACs), adopting Z...
Context. The evolutionary state of blue supergiants is still unknown. Stellar wind mass lo...
Blue stragglers can significantly enhance the spectral energy towards short wavelengths, especially ...
Classical population genetics a priori assigns fitness to alleles without considering molecular or f...
The general problem of pattern formation in biological development is described. One possible type ...
This book gives an overview of atomic diffusion, a fundamental physical process, as applied to all t...
International audienceStellar evolution models of a 0.8 Msolar star (Y=0.2352, Z=0.0001, ?=0.3) have...
We have computed a new grid of evolutionary subdwarf B star (sdB) models from the start of central H...
Context. The pulsation frequencies of early B-type stars cannot be reproduced using stellar models w...
We reexamine the theoretical instability domain of pulsating DB white dwarfs (DBV or V777 Her variab...
We present a new set of nonlinear, convective radial pulsation models for main-sequence stars comput...
This is an electronic version of an article published in The Astrophysical Journal Supplement Series...
Aims. Atomic diffusion, including the effect of radiative accelerations on individual elements, lead...
The evolution of a monoatomic layer, deposited on a substrate, is described by a dynamical model of ...
Context. The physical mechanism leading to the formation of the blue loop in the Hertzsprung–Russell...
We present new grids of evolutionary models for the so-called “Anomalous” Cepheids (ACs), adopting Z...
Context. The evolutionary state of blue supergiants is still unknown. Stellar wind mass lo...
Blue stragglers can significantly enhance the spectral energy towards short wavelengths, especially ...
Classical population genetics a priori assigns fitness to alleles without considering molecular or f...
The general problem of pattern formation in biological development is described. One possible type ...
This book gives an overview of atomic diffusion, a fundamental physical process, as applied to all t...
International audienceStellar evolution models of a 0.8 Msolar star (Y=0.2352, Z=0.0001, ?=0.3) have...
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