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researcher

K. Fujii

13 papers hereh-index 9232 citations19 works total

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

author position
  • first author2
  • middle author9

Across the 11 of 13 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA10
  • astro-ph.HE2
  • astro-ph.SR1
same name
  • K. Fujii — 175 papers, h 47
  • K. Fujii — 89 papers, h 21
  • K. Fujii — 27 papers, h 13
  • K. Fujii — 10 papers, h 7
  • K. Fujii — 10 papers, h 9
  • K. Fujii — 10 papers, h 7

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
20142021
most citedThe two molecular clouds in RCW 38; evidence for formation of the youngest super star cluster in the Milky Way triggered by cloud-cloud collision

114 citations · 319 across the 13 of their papers we have counts for

collaborators
Showing 2015Show all

3 papers · 1 filter

astro-ph.GA2015★ 9 cited

Chemical evolution of the HC3N and N2H+ molecules in dense cores of the Vela C giant molecular cloud complex

Satoshi Ohashi, Ken'ichi Tatematsu, Kosuke Fujii +5

We have observed the HC3N (J=10-9) and N2H+ (J=1-0) lines toward the Vela C molecular clouds with the Mopra 22 m telescope to study chemical characteristics of dense cores. The int…

astro-ph.SR2015★ 114 cited

The two molecular clouds in RCW 38; evidence for formation of the youngest super star cluster in the Milky Way triggered by cloud-cloud collision

Y. Fukui, K. Torii, A. Ohama +13

We present distributions of two molecular clouds having velocities of 2 km s−1 and 14 km s−1 toward RCW 38, the youngest super star cluster in the Milky Way, in the $^{12…

astro-ph.GA2015★ 1 cited

Revealing the Large-Scale Structures of Interstellar Gas Associated with the Magellanic SNR N132D

H. Sano, Y. Fukui, S. Yoshiike +10

We report preliminary results of large-scale distribution toward the Magellanic supernova remnant N132D using Mopra and Chandra archival datasets. We identified a cavity-like CO st…

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