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20052020
most citedDispersal of molecular clouds by ionising radiation

231 citations · 2k across the 33 of their papers we have counts for

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Showing astro-ph.GAShow all

9 papers · 1 filter

astro-ph.GA2017★ 113 cited

Filamentary fragmentation in a turbulent medium

S. D. Clarke, A. P. Whitworth, A. Duarte-Cabral +1

We present the results of smoothed particle hydrodynamic simulations investigating the evolution and fragmentation of filaments that are accreting from a turbulent medium. We show…

astro-ph.GA2016★ 67 cited

Perturbation growth in accreting filaments

Seamus D. Clarke, Anthony P. Whitworth, David A. Hubber

We use smoothed particle hydrodynamic simulations to investigate the growth of perturbations in infinitely long, initially sub-critical but accreting filaments. The growth of these…

astro-ph.GA2014★ 23 cited

First Investigation of the Combined Impact of Ionizing Radiation and Momentum Winds from a Massive Star on a Self-Gravitating Core

Judith Ngoumou, David Hubber, James E. Dale +1

Massive stars shape the surrounding ISM by emitting ionizing photons and ejecting material through stellar winds. To study the impact of the momentum from the wind of a massive sta…

astro-ph.GA2013★ 94 cited

Clumps and triggered star formation in ionised molecular clouds

S. Walch, A. P. Whitworth, T. G. Bisbas +2

Infrared shells and bubbles are ubiquitous in the Galaxy and can generally be associated with HII regions formed around young, massive stars. In this paper, we use high-resolution…

astro-ph.GA2012★ 81 cited

Episodic accretion, protostellar radiative feedback, and their role in low-mass star formation

Dimitris Stamatellos, Anthony P. Whitworth, David A. Hubber

Protostars grow in mass by accreting material through their discs, and this accretion is initially their main source of luminosity. The resulting radiative feedback heats the envir…

astro-ph.GA2012★ 231 cited

Dispersal of molecular clouds by ionising radiation

S. Walch, A. P. Whitworth, T. Bisbas +2

The role of feedback from massive stars is believed to be a key element in the evolution of molecular clouds. We use high-resolution 3D SPH simulations to explore the dynamical eff…