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researcher

C. Clarke

164 papers hereh-index 5711.8k citations304 works total

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

author position
  • sole author4
  • first author10
  • middle author80
  • last author64

Across the 158 of 164 papers where every author was matched, so the position is known.

fields
  • astro-ph57
  • astro-ph.EP55
  • astro-ph.SR41
  • astro-ph.GA10
  • astro-ph.IM1
same name
  • C. Clarke — 88 papers
  • C. Clarke — 64 papers, h 43
  • C. Clarke — 52 papers
  • C. Clarke — 35 papers, h 7
  • C. Clarke — 32 papers, h 58
  • C. Clarke — 17 papers, h 49

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
19932023
most citedCompetitive accretion in embedded stellar cluster

606 citations · 12.5k across the 161 of their papers we have counts for

collaborators
Showing 2018 · astro-ph.SRShow all

3 papers · 2 filters

astro-ph.SR2018★ 121 cited

The FRIED grid of mass loss rates for externally irradiated protoplanetary discs

Thomas J. Haworth, Cathie J. Clarke, Wahidur Rahman +2

We present an open access grid of 3930 calculations of externally evaporating protoplanetary discs. This spans a range of disc sizes (1-400AU), disc masses, UV field strengths (10-…

astro-ph.SR2018★ 42 cited

Evidence of a past disc-disc encounter: HV and DO Tau

Andrew J. Winter, Richard A. Booth, Cathie J. Clarke

Theory and observations suggest that star formation occurs hierarchically due to the fragmentation of giant molecular clouds. In this case we would expect substructure and enhanced…

astro-ph.SR2018★ 179 cited

Protoplanetary disc truncation mechanisms in stellar clusters: comparing external photoevaporation and tidal encounters

Andrew J. Winter, Cathie J. Clarke, Giovanni Rosotti +3

Most stars form and spend their early life in regions of enhanced stellar density. Therefore the evolution of protoplanetary discs (PPDs) hosted by such stars are subject to the in…

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