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researcher

K. Torii

95 papers hereh-index 343.9k citations158 works total

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

author position
  • first author8
  • middle author72
  • last author4

Across the 84 of 95 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA73
  • astro-ph.HE13
  • astro-ph.SR5
  • astro-ph3
  • astro-ph.IM1
same name
  • K. Torii — 47 papers, h 25
  • K. Torii — 7 papers, h 2
  • K. Torii — 5 papers, h 6
  • K. Torii — 2 papers
  • K. Torii — 1 paper
  • K. Torii — 1 paper, h 1

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
20022022
most citedNeutral pion emission from accelerated protons in the supernova remnant W44

229 citations · 4.1k across the 95 of their papers we have counts for

collaborators
Showing 2013 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2013★ 9 cited

Large-scale mapping of the massive star-forming region RCW38 in the [CII] and PAH emission

H. Kaneda, T. Nakagawa, S. K. Ghosh +10

We investigate the large-scale structure of the interstellar medium (ISM) around the massive star cluster RCW38 in the [CII] 158 um line and polycyclic aromatic hydrocarbon (PAH) e…

astro-ph.GA2013★ 164 cited

Molecular Clouds Toward the Super Star Cluster NGC3603; Possible Evidence for a Cloud-Cloud Collision in Triggering the Cluster Formation

Yasuo Fukui, Akio Ohama, Naoki Hanaoka +17

We present new large field observations of molecular clouds with NANTEN2 toward the super star cluster NGC3603 in the transitions 12CO(J=2-1, J=1-0) and 13CO(J=2-1, J=1-0). We sugg…

astro-ph.GA2013★ 55 cited

Non-thermal X-rays and interstellar gas toward the γ-ray supernova remnant RX J1713.7-3946: Evidence for X-ray enhancement around CO and HI clumps

H. Sano, T. Tanaka, K. Torii +18

RX J1713.7-3946 is the most remarkable very-high-energy γ-ray supernova remnant which emits synchrotron X-rays without thermal features. We made a comparative study of CO, HI and X…

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