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20142017
most citedThe Stagger-grid: A grid of 3D stellar atmosphere models - III. The relation to mixing-length convection theory

154 citations · 399 across the 8 of their papers we have counts for

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astro-ph.SR20147 cited

The Stagger-grid: A grid of 3D stellar atmosphere models - VI. Surface appearance of stellar granulation

Zazralt Magic, Martin Asplund

In the surface layers of late-type stars, stellar convection is manifested with its typical granulation pattern due to the presence of convective motions. The resulting photospheri…

astro-ph.SR201419 cited

Planet transit and stellar granulation detection with interferometry

Andrea Chiavassa, Roxanne Ligi, Zazralt Magic +3

Aims. We used realistic three-dimensional (3D) radiative hydrodynamical (RHD) simulations from the Stagger-grid and synthetic images computed with the radiative transfer code Optim…

astro-ph.SR20142 cited

The Stagger-grid: A grid of 3D stellar atmosphere models - V. Fe line shapes, shifts and asymmetries

Zazralt Magic, Remo Collet, Martin Asplund

We present a theoretical study of the effects and signatures of realistic velocity field and atmospheric inhomogeneities associated with convective motions at the surface of cool l…

astro-ph.SR2014150 cited

The Stagger-grid: A grid of 3D stellar atmosphere models - IV. Limb darkening coefficients

Zazralt Magic, Andrea Chiavassa, Remo Collet +1

We compute the emergent stellar spectra from the UV to far infrared for different viewing angles using realistic 3D model atmospheres for a large range in stellar parameters to pre…

astro-ph.SR2014154 cited

The Stagger-grid: A grid of 3D stellar atmosphere models - III. The relation to mixing-length convection theory

Zazralt Magic, Achim Weiss, Martin Asplund

We investigate the relation between 1D atmosphere models that rely on the mixing length theory and models based on full 3D radiative hydrodynamic (RHD) calculations to describe con…