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Y. Ohira

80 papers hereh-index 273.3k citations130 works total

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

author position
  • sole author10
  • first author14
  • middle author33
  • last author19

Across the 76 of 80 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE71
  • astro-ph3
  • astro-ph.CO2
  • astro-ph.IM2
  • physics.plasm-ph2
same name
  • Y. Ohira — 9 papers, h 4
  • Y. Ohira — 2 papers
  • Y. Ohira — 1 paper, h 2
  • Y. Ohira — 1 paper, h 3

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
20072026
most citedDesign Concepts for the Cherenkov Telescope Array

902 citations · 3.2k across the 78 of their papers we have counts for

collaborators
Showing 2018Show all

3 papers · 1 filter

astro-ph.HE2018★ 17 cited

Origin and Impacts of the First Cosmic Rays

Yutaka Ohira, Kohta Murase

Nonthermal phenomena are ubiquitous in the Universe, and cosmic rays (CRs) play various roles in different environments. When, where, and how CRs are first generated since the Big…

astro-ph.HE2018★ 5 cited

A Suzaku X-ray study of the mixed-morphology supernova remnant Kes 69 and searching for its gamma-ray counterpart

Aytap Sezer, Tulun Ergin, Ryo Yamazaki +2

Kes 69 is a mixed-morphology (MM) supernova remnant (SNR) that is known to be interacting with molecular clouds based on 1720 MHz hydroxyl (OH) maser emission observations in the n…

astro-ph.HE2018★ 34 cited

The Transition from Young to Middle-aged Supernova Remnants: Thermal and Nonthermal Aspects of SNR N132D

Aya Bamba, Yutaka Ohira, Ryo Yamazaki +8

Supernova remnants (SNRs) are the primary candidate of Galactic cosmic-ray accelerators. It is still an open issue when and how young SNRs, which typically exhibit strong synchrotr…

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