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researcher

A. Higuchi

35 papers hereh-index 18920 citations47 works total

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

author position
  • first author10
  • middle author19
  • last author1

Across the 30 of 35 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA14
  • astro-ph.EP8
  • astro-ph.SR7
  • astro-ph.IM3
  • astro-ph.CO2
  • astro-ph.HE1
same name
  • A. Higuchi — 59 papers, h 33
  • A. Higuchi — 12 papers, h 12
  • A. Higuchi — 2 papers, h 3
  • A. Higuchi — 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
20092026
most citedFOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45-m telescope (FUGIN) I: Project Overview and Initial Results

205 citations · 1.4k across the 35 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.EP2023★ 1 cited

Dust enrichment and grain growth in a smooth disk around the DG Tau protostar revealed by ALMA triple bands frequency observations

Satoshi Ohashi, Munetake Momose, Akimasa Kataoka +10

Characterizing the physical properties of dust grains in a protoplanetary disk is critical to comprehending the planet formation process. Our study presents ALMA high-resolution ob…

astro-ph.EP2023★ 27 cited

Primordial or Secondary? Testing models of debris disk gas with ALMA

Gianni Cataldi, Yuri Aikawa, Kazunari Iwasaki +13

The origin and evolution of gas in debris disks is still not well understood. Secondary gas production from cometary material or a primordial origin have been proposed. So far, obs…

astro-ph.EP2023★ 4 cited

A Constraint on the Amount of Hydrogen from the CO Chemistry in Debris Disks

Kazunari Iwasaki, Hiroshi Kobayashi, Aya E. Higuchi +1

The faint CO gases in debris disks are easily dissolved into C by UV irradiation, while CO can be reformed via reactions with hydrogen. The abundance ratio of C/CO could thus be a…

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