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G. Williams

3 papers hereh-index 5141 citations24 works total

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

author position
  • first author1
  • middle author1
  • last author1

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

fields
  • astro-ph.GA3
same name
  • G. Williams — 55 papers
  • G. Williams — 19 papers, h 24
  • G. Williams — 10 papers, h 14
  • G. Williams — 6 papers, h 18
  • G. Williams — 5 papers
  • G. Williams — 4 papers, h 31

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 citedAn ALMA study of hub-filament systems I. On the clump mass concentration within the most massive cores

50 citations · 79 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2022★ 8 cited

A Herschel study of G214.5-1.8: a young, cold and quiescent giant molecular filament on the shell of a HI superbubble

S. D. Clarke, A. Sanchez-Monge, G. M. Williams +3

We present an analysis of the outer Galaxy giant molecular filament (GMF) G214.5-1.8 (G214.5) using Herschel data. We find that G214.5 has a mass of ∼ 16,000 M⊙​, yet…

astro-ph.GA2021★ 21 cited

ALMA observations of the Extended Green Object G19.01−0.03: I. A Keplerian disc in a massive protostellar system

Gwenllian M. Williams, Claudia J. Cyganowski, Crystal L. Brogan +6

Using the Atacama Large Millimetre/submillimeter Array (ALMA) and the Karl G. Jansky Very Large Array (VLA), we observed the Extended Green Object (EGO) G19.01−0.03 with sub-arcs…

astro-ph.GA2021★ 50 cited

An ALMA study of hub-filament systems I. On the clump mass concentration within the most massive cores

Michael Anderson, Nicolas Peretto, Sarah E. Ragan +7

The physical processes behind the transfer of mass from parsec-scale clumps to massive-star-forming cores remain elusive. We investigate the relation between the clump morphology a…

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