activity
20052020
most citedEnzo: An Adaptive Mesh Refinement Code for Astrophysics

869 citations · 3.3k across the 34 of their papers we have counts for

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Showing astro-ph.GAShow all

20 papers · 1 filter

astro-ph.GA2018★ 17 cited

The changing GMC population in galaxy interactions

Alex R. Pettitt, Fumi Egusa, Clare L. Dobbs +3

With the advent of modern observational efforts providing extensive giant molecular cloud catalogues, understanding the evolution of such clouds in a galactic context is of prime i…

astro-ph.GA2017★ 1 cited

The Impact of Galactic Disc Environment on Star-Forming Clouds

Ngan K. Nguyen, Alex R. Pettitt, Elizabeth J. Tasker +1

We explore the effect of different galactic disc environments on the properties of star-forming clouds through variations in the background potential in a set of isolated galaxy si…

astro-ph.GA2017★ 30 cited

The effect of photoionising feedback on star formation in isolated and colliding clouds

Kazuhiro Shima, Elizabeth J. Tasker, Christoph Federrath +1

We investigate star formation occurring in idealised giant molecular clouds, comparing structures that evolve in isolation versus those undergoing a collision. Two different collis…

astro-ph.GA2017★ 70 cited

Formation of Massive, Dense Cores by Cloud-Cloud Collisions

Ken Takahira, Kazuhiro Shima, Elizabeth J. Tasker +1

We performed sub-parsec ( 0.014 pc) scale simulations of cloud-cloud collisions of two idealized turbulent molecular clouds (MCs) with different masses in the range of $0.76…

astro-ph.GA2017★ 46 cited

Star formation and ISM morphology in tidally induced spiral structures

Alex R. Pettitt, Elizabeth J. Tasker, James W. Wadsley +2

Tidal encounters are believed to be one of the key drivers of galactic spiral structure in the Universe. Such spirals are expected to produce different morphological and kinematic…

astro-ph.GA2017★ 41 cited

On the effective turbulence driving mode of molecular clouds formed in disc galaxies

Keitaro Jin, Diane M. Salim, Christoph Federrath +3

We determine the physical properties and turbulence driving mode of molecular clouds formed in numerical simulations of a Milky Way-type disc galaxy with parsec-scale resolution. T…