activity
20002025
most citedNumerical simulations of surface convection in a late M-dwarf

106 citations · 563 across the 18 of their papers we have counts for

collaborators

16 papers

astro-ph.SR2025★ 2 cited

Granulation signatures in 3D hydrodynamical simulations: evaluating background model performance using a Bayesian nested sampling framework

Jens R. Larsen, Mia S. Lundkvist, Guy R. Davies +5

Understanding the granulation background signal is of vital importance when interpreting the asteroseismic diagnostics of solar-like oscillators. Various descriptions exist in the…

astro-ph.SR2017★ 18 cited

Three-dimensional hydrodynamical CO5BOLD model atmospheres of red giant stars VI. First chromosphere model of a late-type giant

Sven Wedemeyer, Arunas Kucinskas, Jonas Klevas +1

Although observational data unequivocally point out to the presence of chromospheres in red giant stars, no attempts have been made so far to model them using 3D hydrodynamical mod…

astro-ph.SR2017★ 15 cited

On the computation of eigenfrequencies for equilibrium models including turbulent pressure

T. Sonoi, K. Belkacem, M. -A. Dupret +4

The space-borne missions have provided a wealth of highly accurate data. However, our inability to properly model the upper-most region of solar-like stars prevents us from making…

astro-ph.SR2013★ 45 cited

Stellar granulation as seen in disk-integrated intensity. II. Theoretical scaling relations compared with observations

R. Samadi, K. Belkacem, H. -G. Ludwig +9

A large set of stars observed by CoRoT and Kepler shows clear evidence for the presence of a stellar background, which is interpreted to arise from surface convection, i.e., granul…

astro-ph.SR2012★ 43 cited

3D hydrodynamical CO5BOLD model atmospheres of red giant stars: I. Atmospheric structure of a giant located near the RGB tip

H. -G. Ludwig, A. Kucinskas

We investigate the character and role of convection in the atmosphere of a prototypical red giant located close to the red giant branch (RGB) tip with atmospheric parameters, Teff=…

astro-ph.SR2012★ 22 cited

Three-dimensional magnetohydrodynamic simulations of M-dwarf chromospheres

S. Wedemeyer, H. -G. Ludwig, O. Steiner

We present first results from three-dimensional radiation magnetohydrodynamic simulations of M-type dwarf stars with CO5BOLD. The local models include the top of the convection zon…