most citedModelling the supernova-driven ISM in different environments

171 citations · 445 across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2024

Multiple power-law tails in the density and column-density distribution in contracting star-forming clumps

Todor V. Veltchev, Philipp Girichidis, Lyubov Marinkova +3

We present a numerical study of the evolution of power-law tails (PLTs) in the (column-)density distributions (-PDF, -PDF) in contracting star-forming clumps in primordial ga…

astro-ph.GA201615 cited

The impact of magnetic fields on the chemical evolution of the supernova-driven ISM

Anabele-Linda Pardi, Philipp Girichidis, Thorsten Naab +7

We present three-dimensional magneto-hydrodynamical simulations of the self-gravitating interstellar medium (ISM) in a periodic (256 pc) box with a mean number density of 0.5 c…

astro-ph.GA201617 cited

The turbulent life of dust grains in the supernova-driven, multi-phase interstellar medium

Thomas Peters, Svitlana Zhukovska, Thorsten Naab +6

Dust grains are an important component of the interstellar medium (ISM) of galaxies. We present the first direct measurement of the residence times of interstellar dust in the diff…

astro-ph.GA2016112 cited

The SILCC project --- IV. Impact of dissociating and ionising radiation on the interstellar medium and Halpha emission as a tracer of the star formation rate

Thomas Peters, Thorsten Naab, Stefanie Walch +7

We present three-dimensional radiation-hydrodynamical simulations of the impact of stellar winds, photoelectric heating, photodissociating and photoionising radiation, and supernov…

astro-ph.GA2014

Turbulence in Giant Molecular Clouds: The effect of photoionisation feedback

D. M. Boneberg, J. E. Dale, P. Girichidis +1

Giant Molecular Clouds (GMCs) are observed to be turbulent, but theory shows that without a driving mechanism turbulence should quickly decay. The question arises by which mechanis…

astro-ph.GA2014171 cited

Modelling the supernova-driven ISM in different environments

A. Gatto, S. Walch, M. -M. Mac Low +11

We use hydrodynamical simulations in a periodic box to model the impact of supernova (SN) explosions on the multi-phase interstellar medium (ISM) for initial de…