367 citations · 6.4k across the 103 of their papers we have counts for
6 papers · 1 filter
The GRIFFIN project -- Formation of star clusters with individual massive stars in a simulated dwarf galaxy starburst
Natalia Lahén, Thorsten Naab, Peter H. Johansson +5
We describe a population of young star clusters (SCs) formed in a hydrodynamical simulation of a gas-rich dwarf galaxy merger resolved with individual massive stars at sub-parsec s…
Hot phase generation by supernovae: resolution, chemistry and thermal conduction
Ulrich P. Steinwandel, Benjamin P. Moster, Thorsten Naab +2
Supernovae (SN) generate hot gas in the interstellar medium (ISM), help setting the ISM structure and support the driving of outflows. It is important to resolve the hot gas genera…
The formation of low metallicity globular clusters in dwarf galaxy mergers
Natalia Lahén, Thorsten Naab, Peter H. Johansson +3
We present a hydro-dynamical simulation at sub-parsec and few solar mass resolution of a merger between two gas-rich dwarf galaxies. Our simulation includes a detailed model for th…
X-raying molecular clouds with a short flare: probing statistics of gas density and velocity fields
I. Khabibullin, E. Churazov, R. Sunyaev +3
We take advantage of a set of molecular cloud simulations to demonstrate a possibility to uncover statistical properties of the gas density and velocity fields using reflected emis…
SILCC-Zoom: H and CO-dark gas in molecular clouds -- The impact of feedback and magnetic fields
D. Seifried, S. Haid, S. Walch +2
We analyse the CO-dark molecular gas content of simulated molecular clouds from the SILCC-Zoom project. The simulations reach a resolution of 0.1 pc and include H and CO format…
Determining the presence of characteristic fragmentation length-scales in filaments
S. D. Clarke, G. M. Williams, J. C. Ibáñez-Mejía +1
Theories suggest that filament fragmentation should occur on a characteristic fragmentation length-scale. This fragmentation length-scale can be related to filament properties, suc…