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R. Williams

3 papers hereh-index 452 citations7 works total

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

author position
  • last author1

Across the 1 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA1
  • astro-ph.SR1
  • physics.atom-ph1
same name
  • R. Williams — 184 papers
  • R. Williams — 21 papers, h 27
  • R. Williams — 12 papers
  • R. Williams — 8 papers, h 8
  • R. Williams — 8 papers
  • R. Williams — 6 papers, h 4

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
20162023
most citedThe physical properties of T Pyx as measured by MUSE I. The geometrical distribution of the ejecta and the distance to the remnant

4 citations · 4 across the 1 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2023★ 4 cited

The physical properties of T Pyx as measured by MUSE I. The geometrical distribution of the ejecta and the distance to the remnant

L. Izzo, L. Pasquini, E. Aydi +8

T Pyx is one of the most enigmatic recurrent novae, and it has been proposed as a potential Galactic type-Ia supernova progenitor. Using spatially-resolved data obtained with MUSE,…

physics.atom-ph2017

Thermodynamically-consistent semi-classical ℓ-changing rates

R. J. R. Williams, F. Guzmán, N. R. Badnell +3

We compare the results of the semi-classical (SC) and quantum-mechanical (QM) formalisms for angular-momentum changing transitions in Rydberg atom collisions given by Vrinceanu & F…

astro-ph.GA2016

H, He-like recombination spectra I: l-changing collisions for hydrogen

F. Guzmán, N. R. Badnell, R. J. R. Williams +3

Hydrogen and helium emission lines in nebulae form by radiative recombination. This is a simple process which, in principle, can be described to very high precision. Ratios of He I…

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