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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 2010 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2010★ 193 cited

Modeling CO Emission: I. CO as a Column Density Tracer and the X-Factor in Molecular Clouds

Rahul Shetty, Simon C. Glover, Cornelis P. Dullemond +1

Theoretical and observational investigations have indicated that the abundance of carbon monoxide (CO) is very sensitive to intrinsic properties of the gaseous medium, such as dens…

astro-ph.GA2010★ 45 cited

The Abundance of Molecular Hydrogen and its Correlation with Midplane Pressure in Galaxies: Non-Equilibrium, Turbulent, Chemical Models

Mordecai-Mark Mac Low, Simon C. O. Glover

Observations of spiral galaxies show a strong linear correlation between the ratio of molecular to atomic hydrogen surface density R_mol and midplane pressure. To explain this, we…

astro-ph.GA2010★ 44 cited

A quantification of the non-spherical geometry and accretion of collapsing cores

Rowan J. Smith, Simon C. O. Glover, Ian A. Bonnell +2

We present the first detailed classification of the structures of Class 0 cores in a high resolution simulation of a giant molecular cloud. The simulated cloud contains 10^4 solar…

astro-ph.GA2010

The Effect of Environment on Massive Star Formation

Rowan J Smith, Paul C. Clark, Simon C. O. Glover +2

In this contribution we review our recent numerical work discussing the essential role of the local cluster environment in assembling massive stars. First we show that massive star…

astro-ph.GA2010★ 295 cited

Gravitational fragmentation in turbulent primordial gas and the initial mass function of Population III stars

Paul C. Clark, Simon C. O. Glover, Ralf S. Klessen +1

We report results from numerical simulations of star formation in the early universe that focus on the dynamical behavior of metal-free gas under different initial and environmenta…

astro-ph.GA2010★ 259 cited

On the Relationship Between Molecular Hydrogen and Carbon Monoxide Abundances in Molecular Clouds

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

The most usual tracer of molecular gas is line emission from CO. However, the reliability of that tracer has long been questioned in environments different from the Milky Way. We s…