◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

E. I. Makarenko

1 paper here

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

author position
  • first author1

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

fields
  • astro-ph.HE1
ORCID 0000-0002-9694-1790
same name
  • E. I. Makarenko — 1 paper

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 · 10 across the 1 of their papers we have counts for

collaborators

1 paper

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…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.