68 citations · 175 across the 6 of their papers we have counts for
6 papers
Spatial motion of the Magellanic Clouds. Tidal models ruled out?
Adam Ruzicka, Christian Theis, Jan Palous
Recently, Kallivayalil et al. derived new values of the proper motion for the Large and Small Magellanic Clouds (LMC and SMC, respectively). The spatial velocities of both Clouds a…
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…
Gas stripping in galaxy clusters: a new SPH simulation approach
P. Jachym, J. Palous, J. Koppen +1
The influence of a time-varying ram pressure on spiral galaxies in clusters is explored with a new simulation method based on the N-body SPH/tree code GADGET. We have adapted the c…
Super stellar clusters with a bimodal hydrodynamic solution: an Approximate Analytic Approach
R. Wunsch, S. Silich, J. Palous +1
We look for a simple analytic model to distinguish between stellar clusters undergoing a bimodal hydrodynamic solution from those able to drive only a stationary wind. Clusters in…
Super Massive Star Clusters: From Superwinds to a Cooling Catastrophe and the Re-processing of the Injected Gas
S. Silich, G. Tenorio-Tagle, C. Munoz-Tunon +1
Different hydrodynamic regimes for the gaseous outflows generated by multiple supernovae explosions and stellar winds occurring within compact and massive star clusters are discuss…
Is the dark matter halo of the Milky Way flattened?
A. Ruzicka, J. Palous, Ch. Theis
We performed an extended analysis of the parameter space for the interaction of the Magellanic System with the Milky Way (MW). The varied parameters cover the phase space parameter…