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F. Nakamura

146 papers hereh-index 425.6k citations215 works total

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

author position
  • sole author2
  • first author23
  • middle author90
  • last author14

Across the 129 of 146 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA91
  • astro-ph.SR32
  • astro-ph17
  • astro-ph.IM6
same name
  • F. Nakamura — 28 papers, h 7
  • F. Nakamura — 18 papers, h 17
  • F. Nakamura — 9 papers, h 5
  • F. Nakamura — 5 papers, h 2
  • F. Nakamura — 2 papers, h 1
  • F. Nakamura — 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
19942026
most citedOutflow Feedback Regulated Massive Star Formation in Parsec-Scale Cluster Forming Clumps

387 citations · 7.1k across the 144 of their papers we have counts for

collaborators
Showing 2005Show all

3 papers · 1 filter

astro-ph2005★ 201 cited

Cluster Formation in Protostellar Outflow-Driven Turbulence

Zhi-Yun Li, Fumitaka Nakamura

Most, perhaps all, stars go through a phase of vigorous outflow during formation. We examine, through 3D MHD simulation, the effects of protostellar outflows on cluster formation.…

astro-ph2005★ 136 cited

On the Hydrodynamic Interaction of Shock Waves with Interstellar Clouds. II. The Effect of Smooth Cloud Boundaries on Cloud Destruction and Cloud Turbulence

Fumitaka Nakamura, Christopher F. McKee, Richard I. Klein +1

The effect of smooth cloud boundaries on the interaction of steady planar shock waves with interstellar clouds is studied using a high-resolution local AMR technique with a second-…

astro-ph2005★ 126 cited

Quiescent Cores and the Efficiency of Turbulence-Accelerated, Magnetically Regulated Star Formation

Fumitaka Nakamura, Zhi-Yun Li

The efficiency of star formation, defined as the ratio of the stellar to total (gas and stellar) mass, is observed to vary from a few percent in regions of dispersed star formation…

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