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19982026
most citedThe minimum mass for star formation, and the origin of binary brown dwarfs

162 citations · 1.7k across the 35 of their papers we have counts for

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14 papers · 1 filter

astro-ph2008★ 19 cited

The direction of outflows from filaments : constraints on core formation

S. V. Anathpindika, A. P. Whitworth

Context: It is generally presumed that the outflows from a YSO are directed close to its rotation axis (i.e. along its angular momentum vector and orthogonal to any attendant accre…

astro-ph2007★ 40 cited

Adaptive smoothing lengths in SPH

R. E. Attwood, S. P. Goodwin, A. P. Whitworth

Context: There is a need to improve the fidelity of SPH simulations of self-gravitating gas dynamics. Aims: We remind users of SPH that, if smoothing lengths are adjusted so as to…

astro-ph2006★ 139 cited

Ionisation-induced star formation I: The collect and collapse model

J. E. Dale, I. A. Bonnell, A. P. Whitworth

We conduct Smoothed Particle Hydrodynamics simulations of the `collect and collapse' scenario (Elmegreen and Lada, 1977) for star formation triggered by an expanding HII region. We…

astro-ph2006★ 162 cited

The minimum mass for star formation, and the origin of binary brown dwarfs

A. P. Whitworth, D. Stamatellos

Our first aim is to calculate the minimum mass for Primary Fragmentation in a variety of potential star-formation scenarios, i.e. (i) hierarchical fragmentation of a 3-D medium; (i…

astro-ph2005★ 13 cited

The formation of brown dwarfs

A. P. Whitworth, S. P. Goodwin

We review four mechanisms for forming brown dwarfs: (i) turbulent fragmentation (producing very low-mass prestellar cores); (ii) gravitational instabilities in discs; (iii) dynamic…

astro-ph2005★ 2 cited

Observational characteristics of dense cores with deeply embedded young protostars

D. Stamatellos, A. P. Whitworth, S. P. Goodwin

Class 0 objects, which are thought to be the youngest protostars, are identified in terms of NIR or radio emission and/or the presence of molecular outflows. We present combined hy…