World's Best Scientists 2026 revealed!
Yasuo Fukui

Yasuo Fukui

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Physics
Japan
2026

D-Index & Metrics

Physics

D-Index
135
Citations
67583
World Ranking
469
National Ranking
9

Research.com Recognitions

  • 2026 - Research.com Physics in Japan Leader Award
  • 2023 - Research.com Physics in Japan Leader Award
  • 2022 - Research.com Physics in Japan Leader Award

Overview

Yasuo Fukui is affiliated with Nagoya University in Japan, with a primary research focus in the fields of physics and astronomy. Their publication record includes extensive work in astronomy and astrophysics, nuclear and high energy physics, spectroscopy, atmospheric science, and fluid flow and transfer processes.

The main topics covered in Yasuo Fukui's research comprise:

  • Astrophysics and Star Formation Studies
  • Stellar, planetary, and galactic studies
  • Gamma-ray bursts and supernovae
  • Astrophysics and Cosmic Phenomena
  • Galaxies: Formation, Evolution, Phenomena
  • Astro and Planetary Science
  • Atmospheric Ozone and Climate

Frequent publication venues for this researcher include:

  • The Astrophysical Journal
  • arXiv (Cornell University)
  • Publications of the Astronomical Society of Japan
  • Monthly Notices of the Royal Astronomical Society
  • Zenodo (CERN European Organization for Nuclear Research)

Yasuo Fukui has collaborated extensively with several co-authors including:

  • Hidetoshi Sano
  • Kengo Tachihara
  • Kazuki Tokuda
  • Toshikazu Onishi
  • Kisetsu Tsuge

Some recent papers authored or co-authored by Yasuo Fukui are:

  • Distance of Hi-GAL sources, 2020, Astronomy and Astrophysics
  • Formation of the Musca filament: evidence for asymmetries in the accretion flow due to a cloud-cloud collision, 2020, Springer Link (Chiba Institute of Technology)
  • FRagmentation and Evolution of Dense Cores Judged by ALMA (FREJA). I. Overview: Inner ∼1000 au Structures of Prestellar/Protostellar Cores in Taurus, 2020, The Astrophysical Journal
  • High-mass star formation in Orion B triggered by cloud-cloud collision: Merging molecular clouds in NGC 2024, 2020, Publications of the Astronomical Society of Japan
  • The 30 Doradus Molecular Cloud at 0.4 pc Resolution with the Atacama Large Millimeter/submillimeter Array: Physical Properties and the Boundedness of CO-emitting Structures, 2022, The Astrophysical Journal

Best Publications

  • Observation of top quark production in p̄p collisions with the collider detector at fermilab

    F. Abe;H. Akimoto;A. Akopian;M. G. Albrow

  • The CDF Detector: An Overview

    F. Abe;D. Amidei;G. Apollinari;G. Ascoli

  • Spitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy's Evolution (SAGE) I: Overview and Initial Results

    Margaret Meixner;Karl D. Gordon;Remy Indebetouw;Joseph L. Hora

  • Clouds, filaments and protostars: the Herschel Hi-GAL Milky Way

    S. Molinari;B. Swinyard;J. Bally;M. Barlow

  • Introducing the CTA concept

    B. S. Acharya;M. Actis;T. Aghajani;G. Agnetta

  • Clouds, filaments, and protostars: The Herschel Hi-GAL Milky Way

    S. Molinari;B. Swinyard;J. Bally;M. Barlow

  • Spitzer Survey of the Large Magellanic Cloud: Surveying the Agents of a Galaxy's Evolution (SAGE). I. Overview and Initial Results

    Margaret Meixner;Karl D. Gordon;Remy Indebetouw;Joseph L. Hora

  • Topology of three-jet events in p»p collisions at s=1.8 TeV

    F. Abe;D. Amidei;G. Apollinari;M. Atac

  • Observation of the Bc meson in pp¯ collisions at √s = 1.8 TeV

    F. Abe;H. Akimoto;A. Akopian;M. G. Albrow

  • INCLUSIVE JET CROSS SECTION IN P P COLLISIONS AT S = 1.8 TEV

    F. Abe;H. Akimoto;A. Akopian;M. G. Albrow

  • Hi-GAL: The Herschel Infrared Galactic Plane Survey

    S. Molinari;B. Swinyard;J. Bally;M. Barlow

  • Status of muon collider research and development and future plans

    Charles M. Ankenbrandt;Muzaffer Atac;Bruno Autin;Valeri I. Balbekov

  • Measurement of the antiproton-proton total cross section at s =546 and 1800 GeV

    F. Abe;M. Albrow;D. Amidei;C. Anway-Wiese

  • Planck Early Results: All sky temperature and dust optical depth from Planck and IRAS: Constraints on the "dark gas" in our galaxy

    P. A. R. Ade;N. Aghanim;M. Arnaud

  • The CO-to-H2 Conversion Factor from Infrared Dust Emission across the Local Group

    Adam K. Leroy;Alberto Bolatto;Karl Gordon;Karin Sandstrom

  • Planck early results. XIX. All-sky temperature and dust optical depth from Planck and IRAS. Constraints on the "dark gas" in our Galaxy

    Peter A. R. Ade;N. Aghanim;M. Arnaud;M. Ashdown

  • Charged jet evolution and the underlying event in proton- antiproton collisions at 1.8 TeV

    T. Affolder;H. Akimoto;A. Akopian;M. G. Albrow

  • Discovery of very high energy gamma-ray emission coincident with molecular clouds in the W 28 (G6.4-0.1) field

    F. Aharonian;A.G. Akhperjanian;A.R. Bazer-Bachi;B. Behera

  • Measurement of the Top Quark Mass

    F. Abe;H. Akimoto;A. Akopian;M. G. Albrow

  • Spitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy's Evolution (SAGE). IV. Dust Properties in the Interstellar Medium

    Jean Philippe Bernard;William T. Reach;Deborah Paradis;Margaret Meixner

Frequent Co-Authors

T. Devlin
T. Devlin Rutgers, The State University of New Jersey
K. L. Byrum
K. L. Byrum Argonne National Laboratory
Toshikazu Onishi
Toshikazu Onishi Osaka Metropolitan University
B. Flaugher
B. Flaugher Fermilab
A. Menzione
A. Menzione Scuola Normale Superiore di Pisa
Jay Hauser
Jay Hauser University of California, Los Angeles
J. Yoh
J. Yoh Fermilab
N. S. Lockyer
N. S. Lockyer University of Pennsylvania

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