activity
20142021
most citedModelling the supernova-driven ISM in different environments

171 citations · 253 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2021★ 13 cited

High contrast and resolution near infrared photometry of the core of R136

Zeinab Khorrami, Maud Langlois, Paul C. Clark +8

We present the sharpest and deepest near infrared photometric analysis of the core of R136, a newly formed massive star cluster at the centre of the 30 Doradus star forming region…

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★ 14 cited

Pyroclastic Blowout: Dust Survival in Isolated versus Clustered Supernovae

Sergio Martínez-González, Richard Wünsch, Jan Palouš +3

Following the current debate on the fate of SN-condensed dust grains, here we explore by means of three-dimensional hydrodynamical simulations the interaction of dusty supernova re…

astro-ph.GA2017★ 17 cited

Kinematic clues to the origins of starless HI clouds : dark galaxies or tidal debris ?

R. Taylor, J. I. Davies, P. Jáchym +5

Isolated HI clouds with no optical counterparts are often taken as evidence for galaxy-galaxy interactions, though an alternative hypothesis is that these are primordial 'dark 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…