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E. I. Makarenko

2 papers hereh-index 15 citations3 works total

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

author position
  • middle author1

Across the 1 of 2 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
same name
  • E. I. Makarenko — 4 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

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

10 citations · 11 across the 2 of their papers we have counts for

collaborators

2 papers

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.