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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 2011 · astro-ph.GAShow all

7 papers · 2 filters

astro-ph.GA2011★ 162 cited

TreeCol: a novel approach to estimating column densities in astrophysical simulations

Paul C. Clark, Simon C. O. Glover, Ralf S. Klessen

We present TreeCol, a new and efficient tree-based scheme to calculate column densities in numerical simulations. Knowing the column density in any direction at any location in spa…

astro-ph.GA2011★ 122 cited

Is molecular gas necessary for star formation?

S. C. O. Glover, P. C. Clark

On galactic scales, the surface density of star formation appears to be well correlated with the surface density of molecular gas. This has lead many authors to suggest that there…

astro-ph.GA2011★ 157 cited

Modeling CO Emission: II. The Physical Characteristics that Determine the X factor in Galactic Molecular Clouds

Rahul Shetty, Simon C. Glover, Cornelis P. Dullemond +3

We investigate how the X factor, the ratio of H_2 column density (NH2) to velocity-integrated CO intensity (W), is determined by the physical properties of gas in model molecular c…

astro-ph.GA2011★ 88 cited

The effect of dust cooling on low-metallicity star-forming clouds

Gustavo Dopcke, Simon C. O. Glover, Paul C. Clark +1

The theory for the formation of the first population of stars (Pop III) predicts a IMF composed predominantly of high-mass stars, in contrast to the present-day IMF, which tends to…

astro-ph.GA2011★ 88 cited

Approximations for modelling CO chemistry in GMCs: a comparison of approaches

S. C. O. Glover, P. C. Clark

We examine several different simplified approaches for modelling the chemistry of CO in three-dimensional numerical simulations of turbulent molecular clouds. We compare the differ…

astro-ph.GA2011★ 5 cited

Understanding the physics of the X-factor

S. C. O. Glover, M. -M. Mac Low

We study the relationship between the H2 and CO abundances in simulated molecular clouds using a fully dynamical model of magnetized turbulence coupled to a detailed chemical netwo…