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Dusty supernovae running the thermodynamics of the matter reinserted within young and massive super stellar clusters
Guillermo Tenorio-Tagle, Sergiy Silich, Sergio Martínez-González +3
Following the observational and theoretical evidence that points at core collapse supernovae as major producers of dust, here we calculate the hydrodynamics of the matter reinserte…
Young Stellar Clusters with a Schuster Mass Distribution - I: Stationary Winds
Jan Palous, Richard Wunsch, Sergio Martinez-Gonzalez +3
Hydrodynamic models for spherically-symmetric winds driven by young stellar clusters with a generalized Schuster stellar density profile are explored. For this we use both semi-ana…
On the fate of the matter reinserted within young nuclear stellar clusters
Filiberto Hueyotl-Zahuantitla, Jan Palous, Richard Wunsch +2
This paper presents a hydrodynamical model describing the evolution of the gas reinserted by stars within a rotating young nuclear star cluster (NSC). We explicitly consider the im…
How Significant is Radiation Pressure in the Dynamics of the Gas Around Young Stellar Clusters?
Sergiy Silich, Guillermo Tenorio-Tagle
The impact of radiation pressure on the dynamics of the gas in the vicinity of young stellar clusters is thoroughly discussed. The radiation over the thermal/ram pressure ratio tim…