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R. Yamada

20 papers hereh-index 471 citations21 works total

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

author position
  • first author4
  • middle author15

Across the 19 of 20 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA17
  • astro-ph.HE2
  • astro-ph.IM1
same name
  • R. Yamada — 265 papers
  • R. Yamada — 120 papers, h 46
  • R. Yamada — 11 papers
  • R. Yamada — 10 papers, h 21
  • R. Yamada — 5 papers
  • R. Yamada — 4 papers

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
20192026
most citedHigh-mass star formation in Orion B triggered by cloud-cloud collision: Merging molecular clouds in NGC 2024

35 citations · 110 across the 18 of their papers we have counts for

collaborators
Showing 2021Show all

3 papers · 1 filter

astro-ph.GA2021★ 1 cited

Massive star formation in the Carina nebula complex and Gum 31 -- II. a cloud-cloud collision in Gum 31

Shinji Fujita, Hidetoshi Sano, Rei Enokiya +10

We present the results of analyses of the 12CO (J=1-0), 13CO (J=1-0), and 12CO (J=2-1) emission data toward Gum 31. Three molecular clouds separated in velocity were detected at -2…

astro-ph.GA2021★ 9 cited

Evidence for a Cloud-Cloud Collision in Sh2-233 Triggering the Formation of the High-mass Protostar Object IRAS 05358+3543

R. I. Yamada, Y. Fukui, H. Sano +7

We have carried out a new kinematical analysis of the molecular gas in the Sh2-233 region by using the CO J = 2-1 data taken at ∼0.5 pc resolution. The molecular gas consist…

astro-ph.GA2021★ 1 cited

A Kinematic Analysis of the Giant Molecular Complex W3; Possible Evidence for Cloud-Cloud Collisions that Triggered OB Star Clusters in W3 Main and W3(OH)

R. I. Yamada, H. Sano, K. Tachihara +6

W3 is one of the most outstanding regions of high-mass star formation in the outer solar circle, including two active star-forming clouds, W3 Main and W3(OH). Based on a new analys…

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