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researcher

N. Ohashi

106 papers hereh-index 435.9k citations186 works total

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

author position
  • first author3
  • middle author89
  • last author6

Across the 98 of 106 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR37
  • astro-ph.GA33
  • astro-ph21
  • astro-ph.EP15
same name
  • N. Ohashi — 3 papers, h 4
  • N. Ohashi — 3 papers, h 43
  • N. Ohashi — 2 papers, h 2
  • N. Ohashi — 2 papers, h 1
  • N. Ohashi — 1 paper, h 3
  • N. Ohashi — 1 paper, h 2

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
19992024
most citedDiscovery of Small-Scale Spiral Structures in the Disk of SAO 206462 (HD 135344B): Implications for the Physical State of the Disk from Spiral Density Wave Theory

399 citations · 5.9k across the 106 of their papers we have counts for

collaborators
Showing 2013Show all

3 papers · 1 filter

astro-ph.SR2013★ 154 cited

Local Enhancement of Surface Density in the Protoplanetary Ring Surrounding HD 142527

Misato Fukagawa, Takashi Tsukagoshi, Munetake Momose +15

We report ALMA observations of dust continuum, 13CO J=3--2, and C18O J=3--2 line emission toward a gapped protoplanetary disk around HD 142527. The outer horseshoe-shaped disk show…

astro-ph.GA2013★ 43 cited

Direct Imaging of a Compact Molecular Outflow from a Very Low-luminosity Object; L1521F-IRS

Satoko Takahashi, Nagayoshi Ohashi, Tyler Bourke

We report interferometric observations of the VeLLO L1521F-IRS, in 12CO (2-1) line emission and the 1.3 mm continuum emission, using the Submillimeter Array (SMA). With the 12CO hi…

astro-ph.SR2013★ 95 cited

Unveiling the Evolutionary Sequence from Infalling Envelopes to Keplerian Disks around Low-Mass Protostars

Hsi-Wei Yen, Shigehisa Takakuwa, Nagayoshi Ohashi +1

We performed SMA observations in the C18O (2-1) emission line toward six Class 0 and I protostars, to study rotational motions of their surrounding envelopes and circumstellar mate…

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