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D. A. Williams

3 papers here

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

author position
  • middle author2
  • last author1

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

fields
  • astro-ph2
  • cond-mat.mtrl-sci1
ORCID 0000-0002-7930-9347
same name
  • D. A. Williams — 11 papers
  • D. A. Williams — 4 papers
  • D. A. Williams — 2 papers
  • D. A. Williams — 1 paper

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
20062008
most citedMolecular line intensities as measures of cloud masses - I. Sensitivity of CO emissions to physical parameter variations

131 citations · 280 across the 3 of their papers we have counts for

collaborators
Showing astro-phShow all

2 papers · 1 filter

astro-ph2007★ 46 cited

Molecular tracers of high mass star-formation in external galaxies

E. Bayet, S. Viti, D. A. Williams +1

Hot core molecules should be detectable in external active galaxies out to high redshift. We present here a detailed study of the chemistry of star-forming regions under physical c…

astro-ph2006★ 131 cited

Molecular line intensities as measures of cloud masses - I. Sensitivity of CO emissions to physical parameter variations

T. A. Bell, E. Roueff, S. Viti +1

A reliable estimate of the molecular gas content in galaxies plays a crucial role in determining their dynamical and star-forming properties. However, H2, the dominant molecular sp…

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