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J. Williams

4 papers hereh-index 3165 citations9 works total

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

author position
  • last author3

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

fields
  • astro-ph.GA3
  • astro-ph.SR1
same name
  • J. Williams — 105 papers
  • J. Williams — 49 papers, h 33
  • J. Williams — 46 papers, h 15
  • J. Williams — 40 papers, h 49
  • J. Williams — 26 papers, h 25
  • J. Williams — 21 papers, h 13

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
20112022
most citedSDC13 infrared dark clouds: Longitudinally collapsing filaments?

233 citations · 305 across the 4 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2013★ 51 cited

Pillars and globules at the edges of H ii regions, Confronting Herschel observations and numerical simulations

P. Tremblin, V. Minier, N. Schneider +24

Pillars and globules are present in many high-mass star-forming regions, such as the Eagle nebula (M16) and the Rosette molecular cloud, and understanding their origin will help ch…

astro-ph.GA2013★ 233 cited

SDC13 infrared dark clouds: Longitudinally collapsing filaments?

N. Peretto, G. A. Fuller, Ph. André +11

Formation of stars is now believed to be tightly linked to the dynamical evolution of interstellar filaments in which they form. In this paper we analyze the density structure and…

astro-ph.GA2011★ 11 cited

The JCMT Spectral Legacy Survey: physical structure of the molecular envelope of the high-mass protostar AFGL2591

M. H. D. van der Wiel, F. F. S. van der Tak, M. Spaans +4

The understanding of the formation process of massive stars (>8 Msun) is limited, due to theoretical complications and observational challenges. We investigate the physical structu…

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