Aims. We study the implications of averaging methods with different reference depth scales for 3D hydrodynamical model atmospheres computed with the Stagger-code. The temporally and spatially averaged (hereafter denoted as âŸ̈3Dâ
Between the outer planetary scale and inner (viscous) dissipation scale, the basic equations of the ...
We present a method for performing spectral synthesis based on 1D averages of 3D simulations of conv...
Present grids of stellar atmosphere models are the workhorses in interpreting stellar observations a...
Aims. We present the Stagger-grid, a comprehensive grid of time-dependent, three-dimensional (3D), h...
Theoretical atmosphere models provide the basis for a variety of applications in astronomy. In simpl...
Aims. We study the implications of averaging methods with different reference depth scales for 3D hy...
International audienceContext. The surface structures and dynamics of cool stars are characterised b...
Aims. We compute the emergent stellar spectra from the UV to far infrared for different viewing angl...
Aims. We compute the emergent stellar spectra from the UV to far infrared for different viewing angl...
Context. The use of 3D hydrodynamical simulations of stellar surface convection for model atmosphere...
We have constructed a grid of 3D hydrodynamic simulations of deep convective and line-blanketed atmo...
Stellar evolution codes play a major role in present-day astrophysics, yet they share common issues....
High-precision photometric data from space missions have improved our understanding of stellar granu...
Thanks to high precision photometric data from space missions, our understading of stellar granulati...
During the last couple of years, the number of confirmed exoplanets has increased, especially thanks...
Between the outer planetary scale and inner (viscous) dissipation scale, the basic equations of the ...
We present a method for performing spectral synthesis based on 1D averages of 3D simulations of conv...
Present grids of stellar atmosphere models are the workhorses in interpreting stellar observations a...
Aims. We present the Stagger-grid, a comprehensive grid of time-dependent, three-dimensional (3D), h...
Theoretical atmosphere models provide the basis for a variety of applications in astronomy. In simpl...
Aims. We study the implications of averaging methods with different reference depth scales for 3D hy...
International audienceContext. The surface structures and dynamics of cool stars are characterised b...
Aims. We compute the emergent stellar spectra from the UV to far infrared for different viewing angl...
Aims. We compute the emergent stellar spectra from the UV to far infrared for different viewing angl...
Context. The use of 3D hydrodynamical simulations of stellar surface convection for model atmosphere...
We have constructed a grid of 3D hydrodynamic simulations of deep convective and line-blanketed atmo...
Stellar evolution codes play a major role in present-day astrophysics, yet they share common issues....
High-precision photometric data from space missions have improved our understanding of stellar granu...
Thanks to high precision photometric data from space missions, our understading of stellar granulati...
During the last couple of years, the number of confirmed exoplanets has increased, especially thanks...
Between the outer planetary scale and inner (viscous) dissipation scale, the basic equations of the ...
We present a method for performing spectral synthesis based on 1D averages of 3D simulations of conv...
Present grids of stellar atmosphere models are the workhorses in interpreting stellar observations a...
DOI
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