World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
78
Citations
17120
World Ranking
3196
National Ranking
170

Brunella Nisini 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 Brunella Nisini 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: 434 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.

Brunella Nisini 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 Brunella Nisini 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: 78 D-Index — 15th percentile

15% of scientists in this discipline score the same or lower.

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

Overview

Brunella Nisini is affiliated with the National Institute for Astrophysics in Italy. Their research primarily focuses on physics and astronomy, with a substantial body of work in astrophysics and star formation studies, stellar, planetary, and galactic studies, and astro and planetary science.

The scientist's work covers a range of subfields including astronomy and astrophysics, spectroscopy, instrumentation, atmospheric science, and computational mechanics. Key topics in their research include molecular spectroscopy and structure, gamma-ray bursts and supernovae, as well as astrophysical phenomena and observations.

Their recent publications exemplify the scope of their research activity. Notable papers include:

  • Water in star-forming regions: physics and chemistry from clouds to disks as probed by Herschel spectroscopy (2021, Astronomy and Astrophysics)
  • X-shooter survey of disk accretion in Upper Scorpius (2020, Astronomy and Astrophysics)
  • PENELLOPE: The ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES) (2021, Astronomy and Astrophysics)
  • GIARPS High-resolution Observations of T Tauri stars (GHOsT) (2022, Astronomy and Astrophysics)
  • KMOS study of the mass accretion rate from Class I to Class II in NGC 1333 (2021, Astronomy and Astrophysics)

The scientist frequently collaborates with several co-authors, including:

  • S. Antoniucci
  • T. Giannini
  • C. F. Manara
  • J. M. Alcalá
  • K. Biazzo

Their work is regularly published in multiple prominent venues, with a significant number of publications in:

  • Astronomy and Astrophysics
  • arXiv (Cornell University)
  • The Astrophysical Journal
  • The Astronomical Journal
  • Zenodo (CERN European Organization for Nuclear Research)

Best Publications

  • The ISO Long-Wavelength Spectrometer

    P. E. Clegg;P. A. R. Ade;C. Armand;J.-P. Baluteau

  • Gaps and Rings in an ALMA Survey of Disks in the Taurus Star-forming Region

    Feng Long;Paola Pinilla;Gregory J. Herczeg;Daniel Harsono

  • Water in Star-Forming Regions with the Herschel Space Observatory (WISH): Overview of key program and first results

    E. F. van Dishoeck;L. E. Kristensen;A. O. Benz;E. A. Bergin

  • Water in star-forming regions with the Herschel Space Observatory (WISH). I. Overview of key program and first results

    E. F. van Dishoeck;L. E. Kristensen;A. O. Benz;E. A. Bergin

  • Water in star-forming regions with Herschel (WISH). II. Evolution of 557 GHz 110-101 emission in low-mass protostars

    L. E. Kristensen;E. F. Van Dishoeck;E. A. Bergin;R. Visser

  • X-shooter spectroscopy of young stellar objects in Lupus. Accretion properties of class II and transitional objects

    Juan Manuel Alcala;C. F. Manara;A. Natta;A. Natta;Antonio Frasca

  • Jets and Outflows from Star to Cloud: Observations Confront Theory

    A. Frank;T. P. Ray;S. Cabrit;P. Hartigan

  • Water in star forming regions with Herschel (WISH) III. Far-infrared cooling lines in low-mass young stellar objects

    A. Karska;G. J. Herczeg;E. F. van Dishoeck;S. F. Wampfler

  • H~2 active jets in the near IR as a probe of protostellar evolution

    A. Caratti o Garatti;A. Caratti o Garatti;T. Giannini;B. Nisini;D. Lorenzetti

  • Compact Disks in a High-resolution ALMA Survey of Dust Structures in the Taurus Molecular Cloud

    Feng Long;Gregory J. Herczeg;Daniel Harsono;Paola Pinilla;Paola Pinilla

  • Infrared Emission from Dust Structures Surrounding Herbig Ae/Be Stars

    F. Berrilli;G. Corciulo;G. Ingrosso;D. Lorenzetti

  • A combined optical/infrared spectral diagnostic analysis of the HH1 jet

    B. Nisini;F. Bacciotti;T. Giannini;F. Massi

  • First Detection of Water Vapor in a Pre-stellar Core

    Paola Caselli;Paola Caselli;Eric Keto;Edwin A. Bergin;Mario Tafalla

  • Far-Infrared Investigation of Class 0 Sources: Line Cooling*

    Teresa Giannini;Brunella Nisini;Dario Lorenzetti

  • Recipes for stellar jets: results of combined optical/infrared diagnostics

    L. Podio;F. Bacciotti;B. Nisini;J. Eislöffel

  • 1–2.5 $\mu$m spectra of jets from young stars: Strong $\ion{Fe}{ii}$ emission in HH111, HH240-241 and HH120

    B. Nisini;A. Caratti o Garatti;T. Giannini;D. Lorenzetti

  • Warm SiO gas in molecular bullets associated with protostellar outflows

    B. Nisini;C. Codella;T. Giannini;J. Santiago Garcia

  • Water in star-forming regions with Herschel (WISH) - III. Far-infrared cooling lines in low-mass young stellar objects

    A. Karska;G. J. Herczeg;E. F. van Dishoeck;S. F. Wampfler;S. F. Wampfler

  • Water cooling of shocks in protostellar outflows: Herschel-PACS map of L1157

    B. Nisini;M. Benedettini;C. Codella;T. Giannini

  • X-shooter spectroscopy of young stellar objects in Lupus - Lithium, iron, and barium elemental abundances

    K. Biazzo;A. Frasca;J. M. Alcalá;M. Zusi

Frequent Co-Authors

René Liseau
René Liseau Chalmers University of Technology
E. F. van Dishoeck
E. F. van Dishoeck Leiden University
Emmanuel Caux
Emmanuel Caux Federal University of Toulouse Midi-Pyrénées
F. F. S. van der Tak
F. F. S. van der Tak Netherlands Institute for Space Research
Carsten Dominik
Carsten Dominik University of Amsterdam
Rafael Bachiller
Rafael Bachiller Observatorio Astronómico Nacional de España
Arnold O. Benz
Arnold O. Benz ETH Zurich
David A. Neufeld
David A. Neufeld Johns Hopkins University
Luigi Spinoglio
Luigi Spinoglio National Institute for Astrophysics
Glenn J. White
Glenn J. White The Open University

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