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20002026
most citedSimulations on a Moving Mesh: The Clustered Formation of Population III Protostars

478 citations · 20.2k across the 337 of their papers we have counts for

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Showing 2014 · astro-ph.GAShow all

11 papers · 2 filters

astro-ph.GA2014

Physical Processes in the Interstellar Medium

Ralf S. Klessen, Simon C. O. Glover

Interstellar space is filled with a dilute mixture of charged particles, atoms, molecules and dust grains, called the interstellar medium (ISM). Understanding its physical properti…

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★ 132 cited

Dust and Gas in the Magellanic Clouds from the HERITAGE Herschel Key Project. II. Gas-to-Dust Ratio Variations across ISM Phases

Julia Roman-Duval, Karl Gordon, Margaret Meixner +32

The spatial variations of the gas-to-dust ratio (GDR) provide constraints on the chemical evolution and lifecycle of dust in galaxies. We examine the relation between dust and gas…

astro-ph.GA2014★ 112 cited

Constraining the primordial initial mass function with stellar archaeology

Tilman Hartwig, Volker Bromm, Ralf S. Klessen +1

We present a new near-field cosmological probe of the initial mass function (IMF) of the first stars. Specifically, we constrain the lower-mass limit of the Population III (Pop III…

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★ 185 cited

On the nature of star-forming filaments: I. Filament morphologies

Rowan J. Smith, Simon C. O. Glover, Ralf. S. Klessen

We use a suite of high resolution molecular cloud simulations carried out with the moving mesh code Arepo to explore the nature of star-forming filaments. The simulated filaments a…