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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 2013Show all

7 papers · 1 filter

astro-ph.SR2013★ 70 cited

TOPoS: I. Survey design and analysis of the first sample

E. Caffau, P. Bonifacio, L. Sbordone +14

The metal-weak tail of the metallicity distribution function (MDF) of the Galactic Halo stars contains crucial information on the formation mode of the first generation of stars. T…

astro-ph.GA2013★ 113 cited

Quantifying Observational Projection Effects Using Molecular Cloud Simulations

Christopher N. Beaumont, Stella S. R. Offner, Rahul Shetty +2

The physical properties of molecular clouds are often measured using spectral-line observations, which provide the only probes of the clouds' velocity structure. It is hard, though…

astro-ph.CO2013★ 8 cited

Light from the Cosmic Frontier: Gamma-Ray Bursts

L. Amati, J. -L. Atteia, L. Balazs +41

Gamma-Ray Bursts (GRBs) are the most powerful cosmic explosions since the Big Bang, and thus act as signposts throughout the distant Universe. Over the last 2 decades, these ultra-…

astro-ph.GA2013★ 66 cited

On column density thresholds and the star formation rate

Paul C. Clark, Simon C. O. Glover

We present the results of a numerical study designed to address the question of whether there is a column density threshold for star formation within molecular clouds. We have simu…

astro-ph.GA2013★ 40 cited

Molecular cooling in the diffuse interstellar medium

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

We use a simple one-zone model of the thermal and chemical evolution of interstellar gas to study whether molecular hydrogen (H2) is ever an important coolant of the warm, diffuse…

astro-ph.GA2013★ 64 cited

On the temperature structure of the Galactic Centre cloud G0.253+0.016

Paul C Clark, Simon C. O. Glover, Sarah E. Ragan +2

We present a series of smoothed particle hydrodynamical models of G0.253+0.016 (also known as 'The Brick'), a very dense molecular cloud that lies close to the Galactic Centre. We…