90 citations · 113 across the 3 of their papers we have counts for
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astro-ph2004
Excitation rates of p modes: mass luminosity relation across the HR diagram
R. Samadi, D. Georgobiani, R. Trampedach +3
We compute the rates P at which energy is injected into the p modes for a set of 3D simulations of outer layers of stars. We found that Pmax - the maximum in P - scales as (L/M)^s…
astro-ph1999★ 23 cited
Simulations of Oscillation Modes of the Solar Convection Zone
D. Georgobiani, A. G. Kosovichev, R. Nigam +2
We use the three-dimensional hydrodynamic code of Stein and Nordlund to realistically simulate the upper layers of the solar convection zone in order to study physical characterist…