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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…
Discovery of X-ray emission from young suns in the Small Magellanic Cloud
L. M. Oskinova, W. Sun, C. J. Evans +11
We report the discovery of extended X-ray emission within the young star cluster NGC 602 in the Wing of the Small Magellanic Cloud (SMC) based on observations obtained with the Cha…
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…