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J. Williams

26 papers hereh-index 252k citations79 works total

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

author position
  • middle author16
  • last author5

Across the 21 of 26 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR12
  • astro-ph.EP9
  • astro-ph4
  • astro-ph.GA1
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 — 21 papers, h 13
  • J. Williams — 21 papers, h 11

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
20042022
most citedDiscovery of a planetary-mass companion within the gap of the transition disk around PDS 70

700 citations · 2.2k across the 26 of their papers we have counts for

collaborators
Showing 2021Show all

3 papers · 1 filter

astro-ph.SR2021★ 22 cited

Probing protoplanetary disk evolution in the Chamaeleon II region

M. Villenave, F. Menard, W. R. F. Dent +13

Context. Characterizing the evolution of protoplanetary disks is necessary to improve our understanding of planet formation. Constraints on both dust and gas are needed to determin…

astro-ph.SR2021★ 76 cited

PENELLOPE: the ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES) I. Survey presentation and accretion properties of Orion OB1 and σ-Orionis

C. F. Manara, A. Frasca, L. Venuti +69

The evolution of young stars and disks is driven by the interplay of several processes, notably accretion and ejection of material. Critical to correctly describe the conditions of…

astro-ph.EP2021★ 64 cited

Measuring the ratio of the gas and dust emission radii of protoplanetary disks in the Lupus star-forming region

E. Sanchis, L. Testi, A. Natta +15

We perform a comprehensive demographic study of the CO extent relative to dust of the disk population in the Lupus clouds, in order to find indications of dust evolution and possib…

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