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K. Pilkington

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
same name
  • K. Pilkington — 11 papers, h 8

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

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

219 citations · 453 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2014★ 18 cited

The Role of Feedback in Shaping the Structure of the Interstellar Medium

A. P. Walker, B. K. Gibson, K. Pilkington +5

We present an analysis of the role of feedback in shaping the neutral hydrogen (HI) content of simulated disc galaxies. For our analysis, we have used two realisations of two separ…

astro-ph.GA2012★ 216 cited

Thin disc, Thick Disc and Halo in a Simulated Galaxy

C. B. Brook, G. S. Stinson, B. K. Gibson +8

Within a cosmological hydrodynamical simulation, we form a disc galaxy with sub- components which can be assigned to a thin stellar disc, thick disk, and a low mass stellar halo vi…

astro-ph.GA2012

Metallicity Gradients in Simulated Disk Galaxies

K. Pilkington, B. K. Gibson

The stellar metallicity and abundance ratio gradients from the fiducial late-type galaxy simulation of Stinson et al. (2010) are presented. Over 1-3 scalelengths, gradients are sho…

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.