World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
76
Citations
18798
World Ranking
3339
National Ranking
78

Kenji Bekki publication distribution in Physics in 2026

The chart shows the distribution of publications by all Research.com ranked scientists in the field of Physics in 2026. The highlighted bar marks where Kenji Bekki sits on this spectrum.

103–122 publications: 7 scientists 123–142 publications: 10 scientists 143–162 publications: 31 scientists 163–182 publications: 35 scientists 183–202 publications: 53 scientists 203–222 publications: 81 scientists 223–242 publications: 85 scientists 243–262 publications: 112 scientists 263–282 publications: 114 scientists 283–302 publications: 126 scientists 303–322 publications: 136 scientists 323–342 publications: 162 scientists 343–362 publications: 155 scientists 363–382 publications: 156 scientists 383–402 publications: 134 scientists 403–422 publications: 145 scientists 423–442 publications: 147 scientists 443–462 publications: 131 scientists 463–482 publications: 131 scientists 483–502 publications: 116 scientists 503–522 publications: 106 scientists 523–542 publications: 103 scientists 543–562 publications: 87 scientists 563–582 publications: 84 scientists 583–602 publications: 94 scientists 603–622 publications: 70 scientists 623–642 publications: 76 scientists 643–662 publications: 60 scientists 663–682 publications: 54 scientists 683–702 publications: 60 scientists 703–722 publications: 48 scientists 723–742 publications: 64 scientists 743–762 publications: 48 scientists 763–782 publications: 37 scientists 783–802 publications: 43 scientists 803–822 publications: 34 scientists 823–842 publications: 36 scientists 843–862 publications: 32 scientists 863–882 publications: 32 scientists 883–902 publications: 31 scientists 903–922 publications: 25 scientists 923–942 publications: 15 scientists 943–962 publications: 24 scientists 963–982 publications: 13 scientists 983–1,002 publications: 21 scientists 1,003–1,022 publications: 21 scientists 1,023–1,042 publications: 16 scientists 1,043–1,062 publications: 9 scientists 1,063–1,082 publications: 19 scientists 1,083–1,102 publications: 11 scientists 1,103–1,122 publications: 17 scientists 1,123–1,142 publications: 11 scientists 1,143–1,162 publications: 7 scientists 1,163–1,182 publications: 4 scientists 1,183–1,202 publications: 10 scientists 1,203–1,222 publications: 8 scientists 1,223–1,242 publications: 16 scientists 1,243–1,262 publications: 4 scientists 1,263–1,282 publications: 10 scientists 1,283–1,302 publications: 5 scientists 1,303–1,322 publications: 7 scientists 1,323–1,342 publications: 4 scientists 1,343–1,362 publications: 8 scientists 1,363–1,382 publications: 6 scientists 1,383–1,402 publications: 7 scientists 1,403–1,422 publications: 3 scientists 1,423–1,442 publications: 4 scientists 1,443–1,462 publications: 4 scientists 1,463–1,468 publications: 3 scientists 1,469+ publications: 100 scientists
103 publications 1,469+

This scientist: 430 publications — 44th percentile

44% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 1,469 publications or more.

Kenji Bekki D-index placement in Physics in 2026

The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where Kenji Bekki sits on this spectrum.

70–71 D-Index: 76 scientists 72–73 D-Index: 110 scientists 74–75 D-Index: 143 scientists 76–77 D-Index: 153 scientists 78–79 D-Index: 144 scientists 80–81 D-Index: 167 scientists 82–83 D-Index: 167 scientists 84–85 D-Index: 166 scientists 86–87 D-Index: 132 scientists 88–89 D-Index: 155 scientists 90–91 D-Index: 134 scientists 92–93 D-Index: 137 scientists 94–95 D-Index: 102 scientists 96–97 D-Index: 112 scientists 98–99 D-Index: 110 scientists 100–101 D-Index: 116 scientists 102–103 D-Index: 97 scientists 104–105 D-Index: 103 scientists 106–107 D-Index: 87 scientists 108–109 D-Index: 90 scientists 110–111 D-Index: 67 scientists 112–113 D-Index: 78 scientists 114–115 D-Index: 75 scientists 116–117 D-Index: 67 scientists 118–119 D-Index: 69 scientists 120–121 D-Index: 60 scientists 122–123 D-Index: 59 scientists 124–125 D-Index: 53 scientists 126–127 D-Index: 42 scientists 128–129 D-Index: 41 scientists 130–131 D-Index: 33 scientists 132–133 D-Index: 32 scientists 134–135 D-Index: 45 scientists 136–137 D-Index: 19 scientists 138–139 D-Index: 24 scientists 140–141 D-Index: 28 scientists 142–143 D-Index: 31 scientists 144–145 D-Index: 22 scientists 146–147 D-Index: 20 scientists 148–149 D-Index: 12 scientists 150–151 D-Index: 16 scientists 152–153 D-Index: 24 scientists 154–155 D-Index: 23 scientists 156–157 D-Index: 15 scientists 158–159 D-Index: 15 scientists 160–161 D-Index: 11 scientists 162–163 D-Index: 17 scientists 164–165 D-Index: 12 scientists 166–167 D-Index: 11 scientists 168–169 D-Index: 9 scientists 170–171 D-Index: 9 scientists 172–173 D-Index: 11 scientists 174–175 D-Index: 4 scientists 176–177 D-Index: 8 scientists 178–179 D-Index: 5 scientists 180–181 D-Index: 3 scientists 182–183 D-Index: 4 scientists 184 D-Index: 4 scientists 185+ D-Index: 99 scientists
70 D-Index 185+

This scientist: 76 D-Index — 11th percentile

11% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 185 D-Index or more.

Overview

Kenji Bekki is affiliated with the University of Western Australia in Australia. Their research primarily focuses on the field of Physics and Astronomy, with a significant portion of work dedicated to subfields such as Astronomy and Astrophysics, Instrumentation, and Computer Vision and Pattern Recognition.

The scientist's research themes cover various topics within astrophysics, including stellar, planetary, and galactic studies, galaxies' formation and evolution, as well as astrophysics and star formation studies. Additional topics include gamma-ray bursts and supernovae, advanced vision and imaging, and cosmic phenomena.

Frequent coauthors working with Kenji Bekki include:

  • W. J. Couch
  • Duncan A. Forbes
  • B. Koribalski
  • T. Westmeier
  • K. Lee-Waddell

Kenji Bekki has published in several reputable venues. The most frequent publication venues are:

  • Monthly Notices of the Royal Astronomical Society
  • arXiv (Cornell University)
  • OPAL (Open@LaTrobe) (La Trobe University)
  • Astronomy and Astrophysics
  • The Astrophysical Journal

Representative recent papers authored or co-authored by Kenji Bekki include:

  • Galaxy threshing and the origin of ultra-compact dwarf galaxies in the Fornax cluster, 2024, OPAL (Open@LaTrobe) (La Trobe University)
  • Globular cluster formation from gravitational tidal effects of merging and interacting galaxies, 2024, OPAL (Open@LaTrobe) (La Trobe University)
  • The 2dF galaxy redshift survey: The local E+A galaxy population, 2024, OPAL (Open@LaTrobe) (La Trobe University)

The scientist's body of work spans across numerous papers emphasizing the dynamics and characteristics of galaxies and star formation. This includes investigations into compact dwarf galaxies, globular cluster formation, and galaxy population surveys.

Best Publications

  • Passive spiral formation from halo gas starvation: Gradual transformation into S0s

    Kenji Bekki;Yasuhiro Shioya;Warrick J. Couch

  • Passive Spiral Formation from Halo Gas Starvation: Gradual Transformation into S0s

    Kenji Bekki;Warrick J. Couch;Yasuhiro Shioya

  • Formation of ω Centauri from an ancient nucleated dwarf galaxy in the young Galactic disc

    Kenji Bekki;Kenneth Freeman

  • A class of compact dwarf galaxies from disruptive processes in galaxy clusters

    M. J. Drinkwater;M. D. Gregg;M. D. Gregg;M. Hilker;K. Bekki

  • The VMC Survey - I. Strategy and First Data

    M.-R.L. Cioni;M.-R.L. Cioni;G. Clementini;L. Girardi;R. Guandalini

  • Unequal-Mass Galaxy Mergers and the Creation of Cluster S0 Galaxies

    Kenji Bekki

  • Ram pressure stripping of halo gas in disk galaxies: Implications on galactic star formation in different environments

    Kenji Bekki

  • Galaxy threshing and the formation of ultra-compact dwarf galaxies

    Kenji Bekki;Warrick J. Couch;Drinkwater

  • The origin of the double main sequence in Omega Centauri: Helium enrichment due to gas fueling from its ancient host galaxy ?

    Kenji Bekki;John E. Norris

  • Ram-pressure stripping of halo gas in disc galaxies: implications for galactic star formation in different environments

    Kenji Bekki

  • Galaxy threshing and the origin of ultra-compact dwarf galaxies in the Fornax cluster

    K. Bekki;W. J. Couch;M. J. Drinkwater;Y. Shioya

  • Group-Cluster Merging and the Formation of Starburst Galaxies

    Kenji Bekki

  • GALAXY THRESHING AND THE FORMATION OF ULTRACOMPACT DWARF GALAXIES

    Kenji Bekki;Warrick J. Couch;Michael J. Drinkwater

  • The Tidal Origin of the Magellanic Stream and the Possibility of a Stellar Counterpart

    Jonathan D. Diaz;Jonathan D. Diaz;Kenji Bekki

  • Formation and evolution of the Magellanic Clouds – I. Origin of structural, kinematic and chemical properties of the Large Magellanic Cloud

    Kenji Bekki;Masashi Chiba

  • Galactic star formation enhanced and quenched by ram pressure in groups and clusters

    Kenji Bekki

  • Starbursts from strong compression of galactic molecular clouds due to the high pressure of the intracluster medium

    Kenji Bekki;Warrick J. Couch

  • The Origin of the Double Main Sequence in ω Centauri: Helium Enrichment due to Gas Fueling from Its Ancient Host Galaxy?

    Kenji Bekki;John E. Norris

  • WALLABY – an SKA Pathfinder H i survey

    Bärbel S. Koribalski;Bärbel S. Koribalski;L. Staveley-Smith;T. Westmeier;P. Serra

  • A new formation model for M32: A threshed early-type spiral?

    Kenji Bekki;Warrick J. Couch;Michael Drinkwater;Michael D. Gregg

Frequent Co-Authors

Warrick J. Couch
Warrick J. Couch Swinburne University of Technology
Michael J. Drinkwater
Michael J. Drinkwater University of Queensland
Marcella Marconi
Marcella Marconi National Institute for Astrophysics
Joss Bland-Hawthorn
Joss Bland-Hawthorn University of Sydney
Gerhardt R. Meurer
Gerhardt R. Meurer University of Western Australia
Sarah Brough
Sarah Brough University of New South Wales
Lister Staveley-Smith
Lister Staveley-Smith University of Western Australia
Scott M. Croom
Scott M. Croom University of Sydney
Luca Cortese
Luca Cortese University of Western Australia
Martin A.T. Groenewegen
Martin A.T. Groenewegen Royal Observatory of Belgium

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