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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 2012Show all

4 papers · 1 filter

astro-ph.CO2012★ 46 cited

Radio Mini-Halo Emission from Cosmic Rays in Galaxy Clusters and Heating of the Cool Cores

Yutaka Fujita, Yutaka Ohira

It has been proposed that the cool cores of galaxy clusters are stably heated by cosmic rays (CRs). If this is the case, radio mini-halos, which are often found in the central regi…

astro-ph.HE2012★ 180 cited

Observational signatures of particle acceleration in supernova remnants

E. A. Helder, J. Vink, A. M. Bykov +3

We evaluate the current status of supernova remnants as the sources of Galactic cosmic rays. We summarize observations of supernova remnants, covering the whole electromagnetic spe…

astro-ph.HE2012★ 19 cited

Gamma-ray flare and absorption in Crab Nebula: Lovely TeV-PeV astrophysics

Kazunori Kohri, Yutaka Ohira, Kunihito Ioka

We spectrally fit the GeV gamma-ray flares recently-observed in the Crab Nebula by considering a small blob Lorentz-boosted towards us. We point out that the corresponding inverse-…

astro-ph.HE2012★ 34 cited

Effects of Leakage Neutral Particles on Shocks

Yutaka Ohira

In this paper we investigate effects of neutral particles on shocks propagating into the partially ionized medium. We find that for 120 km/s < u_{sh} < 3000 km/s (u_{sh} is the sho…

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