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researcher

C. G. Few

4 papers here

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

author position
  • first author2
  • middle author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
ORCID 0000-0003-3940-7687
same name
  • C. G. Few — 21 papers, h 15

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
20122016
most citedMetallicity Gradients in Disks: Do Galaxies Form Inside-Out?

219 citations · 311 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2016★ 21 cited

The properties, origin and evolution of stellar clusters in galaxy simulations and observations

C. L. Dobbs, A. Adamo, C. G. Few +16

We investigate the properties and evolution of star particles in two simulations of isolated spiral galaxies, and two galaxies from cosmological simulations. Unlike previous numeri…

astro-ph.GA2016★ 21 cited

Testing Hydrodynamics Schemes in Galaxy Disc Simulations

C. G. Few, C. Dobbs, A. Pettitt +1

We examine how three fundamentally different numerical hydrodynamics codes follow the evolution of an isothermal galactic disc with an external spiral potential. We compare an adap…

astro-ph.GA2014★ 50 cited

Chemodynamics of a Simulated Disc Galaxy: Initial Mass Functions and SNIa Progenitors

C. G. Few, S. Courty, B. K. Gibson +2

We trace the formation and advection of several elements within a cosmological adaptive mesh refinement simulation of an L* galaxy. We use nine realisations of the same initial con…

astro-ph.GA2012★ 219 cited

Metallicity Gradients in Disks: Do Galaxies Form Inside-Out?

K. Pilkington, C. G. Few, B. K. Gibson +13

We examine radial and vertical metallicity gradients using a suite of disk galaxy simulations, supplemented with two classic chemical evolution approaches. We determine the rate of…

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