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20012026
most citedThe SILCC (SImulating the LifeCycle of molecular Clouds) project: I. Chemical evolution of the supernova-driven ISM

367 citations · 2.7k across the 54 of their papers we have counts for

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5 papers · 1 filter

astro-ph2008★ 2 cited

Origin of Star-to-Star Abundance Inhomogeneities in Star Clusters

Jan Palouš, Richard Wünsch, Guillermo Tenorio-Tagle +1

The mass reinserted by young stars of an emerging massive compact cluster shows a bimodal hydrodynamic behaviour. In the inner part of the cluster, it is thermally unstable, while…

astro-ph2008★ 68 cited

Two-Dimensional Hydrodynamic Models of Super Star Clusters with a Positive Star Formation Feedback

R. Wunsch, G. Tenorio-Tagle, J. Palous +1

Using the hydrodynamic code ZEUS, we perform 2D simulations to determine the fate of the gas ejected by massive stars within super star clusters. It turns out that the outcome depe…

astro-ph2006★ 65 cited

On the hydrodynamics of the matter reinserted within superstellar clusters

Guillermo Tenorio-Tagle, Richard Wunsch, Sergiy Silich +1

We present semi-analytical and numerical models, accounting for the impact of radiative cooling on the hydrodynamics of the matter reinserted as strong stellar winds and supernovae…

astro-ph2005★ 25 cited

2-D models of layered protoplanetary discs: I. The ring instability

R. Wunsch, H. Klahr, M. Rozyczka

In this work we use the radiation hydrodynamic code TRAMP to perform a two-dimensional axially symmetric model of the layered disc. Using this model we follow the accumulation of m…

astro-ph2001

The fragmentation of expanding shells: cloud formation rates and masses

J. Palous, R. Wunsch, S. Ehlerova

The gravitational instability of expanding shells is discussed. Linear and nonlinear terms are included in an analytical solution in the static and homogeneous medium. We discuss t…