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researcher

G M Williams

3 papers here

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
ORCID 0000-0001-5933-2147

identity via Semantic Scholar / OpenAlex

most citedThe dynamic centres of infrared-dark clouds and the formation of cores

20 citations · 20 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2024★ 20 cited

The dynamic centres of infrared-dark clouds and the formation of cores

Andrew J. Rigby, Nicolas Peretto, Michael Anderson +7

High-mass stars have an enormous influence on the evolution of the interstellar medium in galaxies, so it is important that we understand how they form. We examine the central clum…

astro-ph.GA2024

GMF G214.5-1.8 as traced by CO: I -- cloud-scale CO freeze-out as a result of a low cosmic-ray ionisation rate

S. D. Clarke, V. A. Makeev, Á. Sánchez-Monge +6

We present an analysis of the outer Galaxy giant molecular filament (GMF) G214.5-1.8 (G214.5) using IRAM 30m data of 12CO, 13CO and C18O. We find that the 12CO…

astro-ph.GA2023

ALMA observations of the Extended Green Object G19.01−0.03: II. A massive protostar with typical chemical abundances surrounded by four low-mass prestellar core candidates

Gwenllian M. Williams, Claudia J. Cyganowski, Crystal L. Brogan +3

We present a study of the physical and chemical properties of the Extended Green Object (EGO) G19.01−0.03 using sub-arcsecond angular resolution Atacama Large Millimeter/submilli…

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