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20082026
most citedSimulations on a Moving Mesh: The Clustered Formation of Population III Protostars

478 citations · 4.7k across the 99 of their papers we have counts for

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Showing 2014Show all

5 papers · 1 filter

astro-ph.GA2014★ 154 cited

The Bones of the Milky Way

Alyssa A. Goodman, Joao Alves, Christopher N. Beaumont +8

The very long and thin infrared dark cloud "Nessie" is even longer than had been previously claimed, and an analysis of its Galactic location suggests that it lies directly in the…

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…

astro-ph.GA2014★ 33 cited

Low-metallicity star formation: Relative impact of metals and magnetic fields

Thomas Peters, Dominik R. G. Schleicher, Rowan J. Smith +2

Low-metallicity star formation poses a central problem of cosmology, as it determines the characteristic mass scale and distribution for the first and second generations of stars f…

astro-ph.GA2014★ 209 cited

CO-dark gas and molecular filaments in Milky Way type galaxies

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

We use the moving mesh code AREPO coupled to a time-dependent chemical network to investigate the formation and destruction of molecular gas in simulated spiral galaxies. This allo…

astro-ph.SR2014★ 33 cited

Line Profiles of Cores within Clusters. III. What is the most reliable tracer of core collapse in dense clusters?

Roxana-Adela Chira, Rowan J. Smith, Ralf S. Klessen +2

Recent observational and theoretical investigations have emphasised the importance of filamentary networks within molecular clouds as sites of star formation. Since such environmen…