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researcher

A. Whitworth

125 papers hereh-index 487k citations280 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author2
  • first author7
  • middle author58
  • last author44

Across the 111 of 125 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA73
  • astro-ph31
  • astro-ph.SR17
  • astro-ph.IM3
  • astro-ph.EP1
same name
  • A. Whitworth — 35 papers, h 14
  • A. Whitworth — 5 papers, h 2
  • A. Whitworth — 2 papers, h 2
  • A. Whitworth — 1 paper, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19982023
most citedThe properties of brown dwarfs and low-mass hydrogen-burning stars formed by disc fragmentation

366 citations · 7.1k across the 125 of their papers we have counts for

collaborators
Showing 2015Show all

4 papers · 1 filter

astro-ph.SR2015★ 83 cited

Star Formation triggered by cloud-cloud collisions

S. K. Balfour, A. P. Whitworth, D. A. Hubber +1

We present the results of SPH simulations in which two clouds, each having mass Mo​​=500M⊙​​ and radius Ro​​=2pc, collide head-o…

astro-ph.SR2015★ 65 cited

Investigating the Global Collapse of Filaments Using Smoothed Particle Hydrodynamics

Seamus D. Clarke, Anthony P. Whitworth

We use Smoothed Particle Hydrodynamic simulations of cold, uniform density, self-gravitating filaments, to investigate their longitudinal collapse timescales; these timescales are…

astro-ph.SR2015★ 28 cited

Are the majority of Sun-like stars single?

A. P. Whitworth, O. Lomax

It has recently been suggested that, in the field, ∼56% of Sun-like stars (0.8M⊙​​≲M⋆​≲1.2M⊙​​) are single. We argue her…

astro-ph.SR2015★ 23 cited

On the effects of solenoidal and compressive turbulence in prestellar cores

O. Lomax, A. P. Whitworth, D. A. Hubber

We present the results of an ensemble of SPH simulations that follow the evolution of prestellar cores for 0.2Myr. All the cores have the same mass, and start with the sa…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.