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20032025
most citedSimulations on a Moving Mesh: The Clustered Formation of Population III Protostars

478 citations · 8.2k across the 106 of their papers we have counts for

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Showing astro-ph.SRShow all

14 papers · 1 filter

astro-ph.SR2025★ 2 cited

The fragmentation of molecular clouds in starburst environments

Matt T. Cusack, Paul C. Clark, Simon C. O. Glover +4

A significant amount of star formation occurs and has occurred in environments unlike the solar neighbourhood. The majority of stars formed closer to the peak of the cosmic star fo…

astro-ph.SR2021★ 2 cited

Extreme adaptive optics astrometry of R136. Searching for high proper motion stars

Zeinab Khorrami, M. Langlois, F. Vakili +9

We compared high-contrast near-infrared images of the core of R136 taken by VLT/SPHERE, in two epochs separated by 3.06 years. For the first time we monitored the dynamics of the d…

astro-ph.SR2021★ 13 cited

High contrast and resolution near infrared photometry of the core of R136

Zeinab Khorrami, Maud Langlois, Paul C. Clark +8

We present the sharpest and deepest near infrared photometric analysis of the core of R136, a newly formed massive star cluster at the centre of the 30 Doradus star forming region…

astro-ph.SR2019★ 5 cited

A Code to Make Your Own Synthetic ObservaTIonS (MYOSOTIS)

Zeinab Khorrami, Pouria Khalaj, Anne S. M. Buckner +10

We introduce our new code MYOSOTIS (Make Your Own Synthetic ObservaTIonS) which is designed to produce synthetic observations from simulated clusters. The code can synthesise obser…

astro-ph.SR2015★ 27 cited

Star formation efficiencies of molecular clouds in a galactic center environment

Erik Bertram, Simon C. O. Glover, Paul C. Clark +1

We use the Arepo moving mesh code to simulate the evolution of molecular clouds exposed to a harsh environment similar to that found in the galactic center (GC), in an effort to un…

astro-ph.SR2014★ 28 cited

A new approach to determine optically thick H2 cooling and its effect on primordial star formation

Tilman Hartwig, Paul C. Clark, Simon C. O. Glover +2

We present a new method for estimating the H2 cooling rate in the optically thick regime in simulations of primordial star formation. Our new approach is based on the TreeCol algor…