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researcher

S. Ohashi

46 papers hereh-index 211.4k citations89 works total

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

author position
  • first author12
  • middle author23
  • last author1

Across the 36 of 46 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA27
  • astro-ph.EP10
  • astro-ph.SR9
same name
  • S. Ohashi — 12 papers, h 5
  • S. Ohashi — 1 paper, h 0
  • S. Ohashi — 1 paper, h 4
  • S. Ohashi — 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
20132026
most citedThe ALMA Survey of 70 μm dark High-mass clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation

207 citations · 1.9k across the 45 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.SR2023

Gravitational instability, spiral substructure, and modest grain growth in a typical protostellar disk: Modeling multi-wavelength dust continuum observation of TMC1A

Wenrui Xu, Satoshi Ohashi, Yusuke Aso +1

Embedded, Class 0/I protostellar disks represent the initial condition for planet formation. This calls for better understandings of their bulk properties and the dust grains withi…

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.SR2023★ 25 cited

FAUST VIII. The protostellar disk of VLA 1623-2417 W and its streamers imaged by ALMA

S. Mercimek, L. Podio, C. Codella +25

More than 50% of solar-mass stars form in multiple systems. It is therefore crucial to investigate how multiplicity affects the star and planet formation processes at the protostel…

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