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researcher

R. Okamoto

12 papers hereh-index 8256 citations16 works total

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

author position
  • first author1
  • middle author11

Across the 12 of 12 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA10
  • astro-ph.HE1
  • astro-ph.SR1
same name
  • R. Okamoto — 32 papers, h 43
  • R. Okamoto — 24 papers, h 19
  • R. Okamoto — 22 papers, h 12
  • R. Okamoto — 3 papers, h 2
  • R. Okamoto — 1 paper, h 2
  • R. Okamoto — 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
20132022
most citedOptically thick HI dominant in the local interstellar medium; an alternative interpretation to "dark gas"

81 citations · 361 across the 12 of their papers we have counts for

collaborators
Showing 2017 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2017★ 5 cited

An Intermediate Velocity HI Cloud Falling to the Galactic Disk; Possible Evidence for Low Metallicity HI Gas Originated Outside the Galactic Disk

Yasuo Fukui, Masako Koga, Shohei Maruyama +6

We found that an intermediate velocity cloud (IVC) IVC 86-36 in HI 21 cm emission shows a head-tail distribution toward the Galactic plane with marked parallel filamentary streamer…

astro-ph.GA2017

Molecular and Atomic Clouds toward the Wolf-Rayet Nebula NGC 2359: Possible Evidence for Isolated High-Mass Star Formation Triggered by a Cloud-Cloud Collision

Hidetoshi Sano, Katsuhiro Hayashi, Rei Enokiya +17

NGC 2359 is an HII region located in the outer Galaxy that contains the isolated Wolf-Rayet (WR) star HD 56925. We present millimeter/submillimeter observations of 12CO(J =…

astro-ph.GA2017★ 27 cited

Synthetic Observations of 21cm HI Line Profiles from Inhomogeneous Turbulent Interstellar HI Gas with Magnetic Field

Yasuo Fukui, Takahiro Hayakawa, Tsuyoshi Inoue +5

We carried out synthetic observations of interstellar atomic hydrogen at 21cm wavelength by utilizing the magneto-hydrodynamical numerical simulations of the inhomogeneous turbulen…

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