World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
85
Citations
23081
World Ranking
2620
National Ranking
1294

T. ten Brummelaar 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 T. ten Brummelaar 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: 516 publications — 58th percentile

58% of scientists in this discipline score the same or lower.

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

T. ten Brummelaar 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 T. ten Brummelaar 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: 85 D-Index — 31st percentile

31% of scientists in this discipline score the same or lower.

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

Overview

T. ten Brummelaar is affiliated with Georgia State University in the United States, specializing in the field of Physics and Astronomy. Their research output spans various subfields including Astronomy and Astrophysics, Instrumentation, Computational Mechanics, Nuclear and High Energy Physics, and Atomic and Molecular Physics, and Optics. The scientist's work primarily focuses on stellar, planetary, and galactic studies, with significant contributions to astrophysics and star formation studies.

Their scholarly output comprises 136 publications in Physics and Astronomy, with notable concentrations across several topics: stellar, planetary, and galactic studies; astrophysics and star formation studies; astronomy and astrophysical research; astro and planetary science; astronomical observations and instrumentation; gamma-ray bursts and supernovae; and adaptive optics and wavefront sensing.

The scientist has published frequently in key academic venues, including:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Astronomy and Astrophysics
  • The Astronomical Journal
  • Monthly Notices of the Royal Astronomical Society

Collaboration has been a consistent feature of ten Brummelaar's career. Frequent co-authors include:

  • Gail Schaefer
  • John D. Monnier
  • Narsireddy Anugu
  • Stefan Kraus
  • Cyprien Lanthermann

Among recent papers authored or co-authored by ten Brummelaar are:

  • "A triple-star system with a misaligned and warped circumstellar disk shaped by disk tearing," 2020, Science
  • "A detailed analysis of the Gl 486 planetary system," 2022, Astronomy and Astrophysics
  • "MYSTIC: a high angular resolution K-band imager at CHARA," 2023, Journal of Astronomical Telescopes Instruments and Systems
  • "Viscous heating in the disk of the outbursting star FU Orionis," 2020, Astronomy and Astrophysics
  • "The Inner Disk of RY Tau: Evidence of Stellar Occultation by the Disk Atmosphere at the Sublimation Rim from K-band Continuum Interferometry," 2020, The Astrophysical Journal

The scientist's research emphasis includes instrumentation, observational techniques, and detailed astrophysical analyses. The body of work reflects engagement with high angular resolution imaging and studies of circumstellar disks, planetary systems, and star formation phenomena.

Best Publications

  • A SURVEY OF STELLAR FAMILIES: MULTIPLICITY OF SOLAR-TYPE STARS

    Deepak Raghavan;Harold A. McAlister;Todd J. Henry;David W. Latham

  • Stellar Diameters and Temperatures II. Main Sequence K & M Stars

    Tabetha S. Boyajian;Kaspar von Braun;Gerard van Belle;Harold A. McAlister

  • Stellar Diameters and Temperatures. II. Main-sequence K- and M-stars

    Tabetha S. Boyajian;Kaspar Von Braun;Gerard Van Belle;Harold A. McAlister

  • First Results from the CHARA Array. II. A Description of the Instrument

    T. A. ten Brummelaar;H. A. McAlister;S. T. Ridgway;W. G. Bagnuolo

  • First Results from the CHARA Array. II. A Description of the Instrument

    T. A. ten Brummelaar;H. A. McAlister;S. T. Ridgway;W. G. Bagnuolo

  • ICCD Speckle Observations of Binary Stars. XIX. An Astrometric/Spectroscopic Survey of O Stars

    Brian D. Mason;Douglas R. Gies;William I. Hartkopf;William G. Bagnuolo

  • Imaging the Surface of Altair

    John D. Monnier;M. Zhao;E. Pedretti;N. Thureau

  • Stellar Diameters and Temperatures III. Main Sequence A, F, G, & K Stars: Additional high-precision measurements and empirical relations

    Tabetha S. Boyajian;Kaspar von Braun;Gerard van Belle;Chris Farrington

  • Fundamental Properties of Stars using Asteroseismology from Kepler & CoRoT and Interferometry from the CHARA Array

    D. Huber;M. J. Ireland;T. R. Bedding;I. M. Brandão

  • Stellar Diameters and Temperatures I. Main Sequence A, F, & G Stars

    Tabetha S. Boyajian;Harold A. McAlister;Gerard van Belle;Douglas R. Gies

  • STELLAR DIAMETERS AND TEMPERATURES. III. MAIN-SEQUENCE A, F, G, AND K STARS: ADDITIONAL HIGH-PRECISION MEASUREMENTS AND EMPIRICAL RELATIONS

    Tabetha S. Boyajian;Tabetha S. Boyajian;Kaspar von Braun;Kaspar von Braun;Gerard van Belle;Chris Farrington

  • Fundamental properties of stars using asteroseismology from Kepler and CoRoT and interferometry from the CHARA Array

    D. Huber;D. Huber;M. J. Ireland;M. J. Ireland;M. J. Ireland;T. R. Bedding;I. M. Brandão

  • STELLAR DIAMETERS AND TEMPERATURES. I. MAIN-SEQUENCE A, F, AND G STARS

    Tabetha S. Boyajian;Harold A. McAlister;Gerard van Belle;Douglas R. Gies

  • First Results from the CHARA Array. VII. Long-Baseline Interferometric Measurements of Vega Consistent with a Pole-On, Rapidly Rotating Star

    J. P. Aufdenberg;A. Mérand;V. Coudé du Foresto;Olivier Absil

  • First Results from the CHARA Array. I. An Interferometric and Spectroscopic Study of the Fast Rotator α Leonis (Regulus)

    H. A. McAlister;T. A. ten Brummelaar;D. R. Gies;D. R. Gies;W. Huang;W. Huang

  • First Resolved Images of the Eclipsing and Interacting Binary β Lyrae

    M. Zhao;D. Gies;J. D. Monnier;N. Thureau

  • Search for Faint Companions to Nearby Solar-like Stars using the Adaptive Optics System at Mount Wilson Observatory*

    Nils H. Turner;Theo A. ten Brummelaar;Harold A. McAlister;Brian D. Mason

  • Long-baseline interferometric multiplicity survey of the Sco-Cen OB association

    Aaron C. Rizzuto;Michael Ireland;Michael Ireland;James G Robertson;Y Kok

  • Adaptive Optics Photometry and Astrometry of Binary Stars. II. A Multiplicity Survey of B Stars

    Lewis C. Roberts;Nils H. Turner;Theo A. ten Brummelaar

  • ICCD Speckle Observations of Binary Stars. XXII. A Survey of Wolf-Rayet Starsfor Close Visual Companions

    William I. Hartkopf;Brian D. Mason;Douglas R. Gies;Theo ten Brummelaar;Theo ten Brummelaar;Theo ten Brummelaar

Frequent Co-Authors

Nils H. Turner
Nils H. Turner Georgia State University
Harold A. McAlister
Harold A. McAlister Georgia State University
John D. Monnier
John D. Monnier University of Michigan–Ann Arbor
Pierre Kervella
Pierre Kervella Université Paris Cité
Michael J. Ireland
Michael J. Ireland Australian National University
Peter G. Tuthill
Peter G. Tuthill University of Sydney
David R. Ciardi
David R. Ciardi California Institute of Technology
Daniel Huber
Daniel Huber University of Hawaii at Manoa
David H. Berger
David H. Berger Harvard University
Grzegorz Pietrzyński
Grzegorz Pietrzyński Polish Academy of Sciences

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