activity
20022025
most citedThe SILCC (SImulating the LifeCycle of molecular Clouds) project: I. Chemical evolution of the supernova-driven ISM

367 citations · 6.4k across the 103 of their papers we have counts for

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Showing 2018Show all

13 papers · 1 filter

astro-ph.GA2018★ 24 cited

Dust charge distribution in the interstellar medium

Juan C. Ibáñez-Mejía, Stefanie Walch, Alexei V. Ivlev +3

We investigate the equilibrium charge distribution of dust grains in the interstellar medium (ISM). Our treatment accounts for collisional charging by electrons and ions, photoelec…

astro-ph.GA2018★ 31 cited

On the resolution requirements for modelling molecular gas formation in solar neighbourhood conditions

P. R. Joshi, S. Walch, D. Seifried +3

The formation of molecular hydrogen (H) and carbon monoxide (CO) is sensitive to the volume and column density distribution of the turbulent interstellar medium. In this paper,…

astro-ph.SR2018★ 14 cited

Evolution of Hubble wedges in episodic protostellar outflows

P. F. Rohde, S. Walch, D. Seifried +2

Young low-mass protostars undergo short phases of high accretion and outburst activity leading to lumpy outflows. Recent observations have shown that the position-velocity and mass…

astro-ph.GA2018★ 56 cited

SILCC-ZOOM: The early impact of ionizing radiation on forming molecular clouds

Sebastian Haid, Stefanie Walch, Daniel Seifried +3

As part of the SILCC-ZOOM project we present our first sub-parsec resolution radiation-hydrodynamic simulations of two molecular clouds self-consistently forming from a turbulent,…

astro-ph.GA2018★ 38 cited

Synthetic [CII] emission maps of a simulated molecular cloud in formation

A. Franeck, S. Walch, D. Seifried +10

The C ion is an important coolant of interstellar gas, and so the [CII] fine structure line is frequently observed in the interstellar medium. However, the physical and chemi…

astro-ph.GA2018★ 69 cited

The SILCC project - V. The impact of magnetic fields on the chemistry and the formation of molecular clouds

Philipp Girichidis, Daniel Seifried, Thorsten Naab +5

Magnetic fields are ubiquitously observed in the interstellar medium (ISM) of present-day star-forming galaxies with dynamically relevant energy densities. Using three-dimensional…