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researcher

H. Kaneko

47 papers hereh-index 15808 citations71 works total

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

author position
  • first author6
  • middle author33
  • last author6

Across the 45 of 47 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA42
  • astro-ph.CO3
  • astro-ph.SR2
same name
  • H. Kaneko — 13 papers, h 8
  • H. Kaneko — 6 papers, h 3
  • H. Kaneko — 3 papers, h 31
  • H. Kaneko — 2 papers, h 9
  • H. Kaneko — 2 papers, h 8
  • H. Kaneko — 2 papers, 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
20092026
most citedBreakdown of Kennicutt-Schmidt Law at GMC Scales in M33

167 citations · 1.1k across the 47 of their papers we have counts for

collaborators
Showing 2018Show all

3 papers · 1 filter

astro-ph.GA2018★ 9 cited

Discovery of a Molecular Collision Front in Interacting Galaxies NGC 4567/4568 with ALMA

Hiroyuki Kaneko, Nario Kuno, Takayuki R. Saitoh

We present results of 12CO(J = 1-0) imaging observations of NGC 4567/4568, a galaxy pair in a close encounter, with Atacama Large Millimetre/submillimetre Array. For the first…

astro-ph.SR2018★ 24 cited

Chemical Diversity in Three Massive Young Stellar Objects associated with 6.7 GHz CH3​OH Masers

Kotomi Taniguchi, Masao Saito, Liton Majumdar +8

We have carried out observations in the 42−46 and 82−103 GHz bands with the Nobeyama 45-m radio telescope, and in the 338.2−339.2 and 348.45−349.45 GHz bands with the ASTE…

astro-ph.GA2018★ 24 cited

Dense molecular gas in the starburst nucleus of NGC 1808

Dragan Salak, Yuto Tomiyasu, Naomasa Nakai +3

Dense molecular gas tracers in the central 1 kpc region of the superwind galaxy NGC 1808 have been imaged by ALMA at a resolution of 1" (~50 pc). Integrated intensities and line in…

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