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P. Williams

4 papers hereh-index 226 citations11 works total

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

author position
  • sole author1
  • first author1
  • last author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR4
same name
  • P. Williams — 50 papers, h 23
  • P. Williams — 31 papers, h 16
  • P. Williams — 18 papers, h 13
  • P. Williams — 14 papers, h 5
  • P. Williams — 10 papers, h 6
  • P. Williams — 9 papers, h 9

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
20112021
most citedThe orbit and stellar masses of the archetype colliding-wind binary WR 140

39 citations · 45 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2021★ 5 cited

The episodic dust-making Wolf-Rayet star HD 38030 in the Large Magellanic Cloud

Peredur M. Williams, Nidia I. Morrell, Konstantina Boutsia +1

Mid-infrared photometry of the Wolf-Rayet star HD 38030 in the Large Magellanic Cloud from the NEOWISE-R mission show it to have undergone a dust-formation episode in 2018 and the…

astro-ph.SR2021★ 39 cited

The orbit and stellar masses of the archetype colliding-wind binary WR 140

Joshua D. Thomas, Noel D. Richardson, J. J. Eldridge +33

We present updated orbital elements for the Wolf-Rayet (WR) binary WR\,140 (HD\,193793; WC7pd + O5.5fc). The new orbital elements were derived using previously published measuremen…

astro-ph.SR2017

Observation of a Deep Visual "Eclipse" in the WC9-Type Wolf-Rayet Star, WR 76

Rod Stubbings, Peredur Williams

The WC9-Type Wolf-Rayet star WR 76 is one of the most prolific dust makers identified from its infrared emission. WR 76 experienced a deep fading eclipse in 2016. The ~3.1 magnitud…

astro-ph.SR2011★ 1 cited

WR 140 in the Infrared

Peredur Williams

Observations in the infrared have played a significant role in the development of our understanding of WR140. Two sets of observations are described here: the changing profile of t…

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