8 citations · 22 across the 5 of their papers we have counts for
5 papers
Simulations of pre-supernova feedback in spherical clouds
Michalis Kourniotis, Richard Wünsch, Sergio Martínez-González +3
We present a one-dimensional radiation-hydrodynamic model of a spherically symmetric cloud evolving under the influence of the self-gravity and the feedback from a star cluster for…
Flash-light on the Ring: hydrodynamic simulations of expandingsupernova shells near supermassive black holes
B. Barna, J. Palouš, S. Ehlerová +3
The way supermassive black holes (SMBH) in galactic centers accumulate their mass is not completely determined. At large scales, it is governed by galactic encounters, mass inflows…
Impact of the external radiation field on the structure and evolution of supernova remnants
Mario Romero, Yago Ascasibar, Jan Palouš +2
We carry out 1D hydrodynamical simulations of the evolution of a spherically symmetric supernova remnant (SNR) subject to an external radiation field (ERF) that influences the cool…
Simulating the evolution of optically dark HI clouds in the Virgo cluster : will no-one rid me of this turbulent sphere ?
Rhys Taylor, Richard Wünsch, Jan Palouš
Most detected neutral atomic hydrogen (HI) at low redshift is associated with optically bright galaxies. However, a handful of HI clouds are known which appear to be optically dark…
The Evolution of Galaxies
Jan Palouš
The evolution of galaxies results from a combination of internal and external processes. The star formation is an internal process transforming cold and dense cores of molecular cl…