activity
20142023
most citedModelling the supernova-driven ISM in different environments

171 citations · 343 across the 6 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2023★ 5 cited

A deep-learning approach to the 3D reconstruction of dust density and temperature in star-forming regions

Victor F. Ksoll, Stefan Reissl, Ralf S. Klessen +7

Aims: We introduce a new deep-learning approach for the reconstruction of 3D dust density and temperature distributions from multi-wavelength dust emission observations on the scal…

astro-ph.GA2022★ 37 cited

The Galactic dynamics revealed by the filamentary structure in atomic hydrogen emission

Juan D. Soler, Marc-Antoine Miville-Deschênes, Sergio Molinari +13

We present a study of the filamentary structure in the atomic hydrogen (HI) emission at the 21 cm wavelength toward the Galactic plane using the observations in the HI4PI survey. U…

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.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.GA2014★ 125 cited

Understanding star formation in molecular clouds I. Effects of line-of-sight contamination on the column density structure

N. Schneider, V. Ossenkopf, T. Csengeri +6

Column-density maps of molecular clouds are one of the most important observables in the context of molecular cloud- and star-formation (SF) studies. With the Herschel satellite it…