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20132016
most citedThe SILCC (SImulating the LifeCycle of molecular Clouds) project: I. Chemical evolution of the supernova-driven ISM

367 citations · 1.6k across the 12 of their papers we have counts for

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11 papers · 1 filter

astro-ph.GA2016★ 15 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.GA2016★ 112 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.GA2016★ 207 cited

The SILCC project: III. Regulation of star formation and outflows by stellar winds and supernovae

A. Gatto, S. Walch, T. Naab +9

We study the impact of stellar winds and supernovae on the multi-phase interstellar medium using three-dimensional hydrodynamical simulations carried out with FLASH. The selected g…

astro-ph.GA2016★ 72 cited

Gas Loss by Ram Pressure Stripping and Internal Feedback From Low Mass Milky Way Satellites

Andrew Emerick, Mordecai-Mark Mac Low, Jana Grcevich +1

The evolution of dwarf satellites of the Milky Way is affected by the combination of ram pressure and tidal stripping, and internal feedback from massive stars. We investigate gas…

astro-ph.GA2016★ 72 cited

Supernova-blast waves in wind-blown bubbles, turbulent, and power-law ambient media

Sebastian Haid, Stefanie Walch, Thorsten Naab +3

Supernova (SN) blast waves inject energy and momentum into the interstellar medium (ISM), control its turbulent multiphase structure and the launching of galactic outflows. Accurat…

astro-ph.GA2015★ 23 cited

Impact of supernova and cosmic-ray driving on the surface brightness of the galactic halo in soft X-rays

Thomas Peters, Philipp Girichidis, Andrea Gatto +7

The halo of the Milky Way contains a hot plasma with a surface brightness in soft X-rays of the order erg cm s deg. The origin of this gas is unclear…

astro-ph.GA2015★ 204 cited

Launching cosmic-ray-driven outflows from the magnetized interstellar medium

Philipp Girichidis, Thorsten Naab, Stefanie Walch +10

We present a hydrodynamical simulation of the turbulent, magnetized, supernova (SN)-driven interstellar medium (ISM) in a stratified box that dynamically couples the injection and…

astro-ph.GA2015★ 233 cited

The SILCC (SImulating the LifeCycle of molecular Clouds) project - II. Dynamical evolution of the supernova-driven ISM and the launching of outflows

Philipp Girichidis, Stefanie Walch, Thorsten Naab +8

The SILCC project (SImulating the Life-Cycle of molecular Clouds) aims at a more self-consistent understanding of the interstellar medium (ISM) on small scales and its link to gala…

astro-ph.GA2014★ 367 cited

The SILCC (SImulating the LifeCycle of molecular Clouds) project: I. Chemical evolution of the supernova-driven ISM

S. K. Walch, P. Girichidis, T. Naab +7

The SILCC project (SImulating the Life-Cycle of molecular Clouds) aims at a more self-consistent understanding of the interstellar medium (ISM) on small scales and its link to gala…

astro-ph.GA2014★ 171 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…

astro-ph.GA2013★ 134 cited

Unveiling the corona of the Milky Way via ram-pressure stripping of dwarf satellites

A. Gatto, F. Fraternali, J. I. Read +3

The spatial segregation between dSphs and dIrrs in the Local Group has long been regarded as evidence of an interaction with their host galaxies. In this paper, we assume that ram-…