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researcher

Pierre Nürnberger

1 paper here

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

author position
  • middle author1

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

fields
  • astro-ph.HE1
ORCID 0000-0003-4384-3115

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…

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