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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 2005Show all

4 papers · 1 filter

astro-ph2005★ 79 cited

The photometric evolution of FU Orionis objects: disc instability and wind-envelope interaction

C. Clarke, G. Lodato, S. Y. Melnikov +1

We present the results of a photometric monitoring campaign of three well studied FU Orionis systems (FU Orionis, V1057 Cygni and V1515 Cygni) undertaken at Maidanak Observatory be…

astro-ph2005★ 96 cited

The Differential Lifetimes of Protostellar Gas and Dust Disks

Taku Takeuchi, C. J. Clarke, D. N. C. Lin

We construct a protostellar disk model that takes into account the combined effect of viscous evolution, photoevaporation and the differential radial motion of dust grains and gas.…

astro-ph2005★ 197 cited

Photoionising feedback in star cluster formation

J. E. Dale, I. A. Bonnell, C. J. Clarke +1

We present the first ever hydrodynamic calculations of star cluster formation that incorporate the effect of feedback from ionising radiation. In our simulations, the ionising sour…

astro-ph2005★ 152 cited

Statistical Confirmation of a Stellar Upper Mass Limit

M. S. Oey, C. J. Clarke

We derive the expectation value for the maximum stellar mass (m_max) in an ensemble of N stars, as a function of the IMF upper-mass cutoff (m_up) and N. We statistically demonstrat…

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