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Hiromasa Suzuki

15 papers here

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

author position
  • first author4
  • middle author3

Across the 7 of 15 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE13
  • astro-ph.GA1
  • astro-ph.IM1
ORCID 0000-0002-8152-6172
same name
  • Hiromasa Suzuki — 5 papers, h 7
  • Hiromasa Suzuki — 4 papers
  • Hiromasa Suzuki — 2 papers, h 11
  • Hiromasa Suzuki — 1 paper
  • Hiromasa Suzuki — 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

activity
20222024
most citedA deep spectromorphological study of the γ-ray emission surrounding the young massive stellar cluster Westerlund 1

50 citations · 170 across the 15 of their papers we have counts for

collaborators

2 papers

astro-ph.HE2022★ 8 cited

Particle acceleration controlled by ambient density in the southwestern rim of RCW 86

Hiromasa Suzuki, Satoru Katsuda, Takaaki Tanaka +3

Particle acceleration physics at supernova remnant (SNR) shocks is one of the most intriguing problems in astrophysics. SNR RCW~86 provides a suitable environment for understanding…

astro-ph.HE2022★ 50 cited

A deep spectromorphological study of the γ-ray emission surrounding the young massive stellar cluster Westerlund 1

F. Aharonian, H. Ashkar, M. Backes +156

Young massive stellar clusters are extreme environments and potentially provide the means for efficient particle acceleration. Indeed, they are increasingly considered as being res…

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