activity
20152025
most citedFilamentary fragmentation in a turbulent medium

113 citations · 844 across the 31 of their papers we have counts for

collaborators
Showing 2018Show all

6 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★ 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★ 85 cited

Synthetic CO observations of fibrous filaments: the problems of mapping from PPV to PPP

S. D. Clarke, A. P. Whitworth, R. L. Spowage +5

Molecular-line observations of filaments in star-forming regions have revealed the existence of elongated coherent features within the filaments; these features are termed fibres.…

astro-ph.GA2018★ 18 cited

J plots: a new method for characterizing structures in the interstellar medium

S. E. Jaffa, A. P. Whitworth, S. D. Clarke +1

Large scale surveys have brought about a revolution in astronomy. To analyse the resulting wealth of data, we need automated tools to identify, classify, and quantify the important…