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Cited article:

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Coupling 1D stellar evolution with 3D-hydrodynamical simulations on-the-fly II: stellar evolution and asteroseismic applications

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Mending the structural surface effect of 1D stellar structure models with non-solar metallicities based on interpolated 3D envelopes

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Analysis of surface effect on solar-like oscillation frequencies using 3D hydrodynamical models

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Damping rates and frequency corrections of Kepler LEGACY stars

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Bayesian inference of stellar parameters based on 1D stellar models coupled with 3D envelopes

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Stellar models with calibrated convection and temperature stratification from 3D hydrodynamics simulations

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Improved Calibration of the Radii of Cool Stars Based on 3D Simulations of Convection: Implications for the Solar Model

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Coupling 1D stellar evolution with 3D-hydrodynamical simulations on the fly – I. A new standard solar model

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The asteroseismic surface effect from a grid of 3D convection simulations – I. Frequency shifts from convective expansion of stellar atmospheres

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Theoretical oscillation frequencies for solar-type dwarfs from stellar models with 〈3D〉-atmospheres

Andreas Christ Sølvsten Jørgensen, Achim Weiss, Jakob Rørsted Mosumgaard, Victor Silva Aguirre and Christian Lundsgaard Sahlholdt
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