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researcher

S. Clarke

32 papers hereh-index 13466 citations42 works total

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

author position
  • first author9
  • middle author20
  • last author1

Across the 30 of 32 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA24
  • astro-ph.SR6
  • astro-ph.HE2
same name
  • S. Clarke — 20 papers, h 34
  • S. Clarke — 15 papers, h 25
  • S. Clarke — 6 papers, h 11
  • S. Clarke — 6 papers, h 1
  • S. Clarke — 3 papers, h 3
  • S. Clarke — 2 papers, h 2

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
20152025
most citedFilamentary fragmentation in a turbulent medium

113 citations · 844 across the 31 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

2 papers · 1 filter

astro-ph.HE2024★ 1 cited

How do supernova remnants cool? II. Machine learning analysis of supernova remnant simulations

P. Smirnova, E. I. Makarenko, S. D. Clarke +4

About 15%-60% of all supernova remnants are estimated to interact with dense molecular clouds. In these high density environments, radiative losses are significant. The cooling rad…

astro-ph.HE2023★ 10 cited

How do supernova remnants cool? -- I. Morphology, optical emission lines, and shocks

Ekaterina I. Makarenko, Stefanie Walch, Seamus D. Clarke +4

Supernovae (SNe) inject ∼1051 erg in the interstellar medium, thereby shocking and heating the gas. A substantial fraction of this energy is later lost via radiative cooli…

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