World's Best Scientists 2026 revealed!
William R. Forman

William R. Forman

D-Index & Metrics

Physics

D-Index
143
Citations
70415
World Ranking
370
National Ranking
211

Overview

What is he best known for?

The fields of study he is best known for:

  • Astronomy
  • Astrophysics
  • Galaxy

His main research concerns Astrophysics, Astronomy, Galaxy cluster, Galaxy and Surface brightness. His work in Cooling flow, Redshift, Radio galaxy, Intracluster medium and Active galactic nucleus are all subfields of Astrophysics research. His Cooling flow course of study focuses on Supermassive black hole and Accretion.

His Galaxy cluster study incorporates themes from Cosmic microwave background and Dark matter. The study incorporates disciplines such as Amplitude, Jet and Virial mass in addition to Surface brightness. His research investigates the connection between ROSAT and topics such as Cosmology that intersect with problems in X-ray.

His most cited work include:

  • Erratum: "Chandra Sample of Nearby Relaxed Galaxy Clusters: Mass, Gas Fraction, and Mass-Temperature Relation" (1204 citations)
  • Chandra sample of nearby relaxed galaxy clusters: mass, gas fraction, and mass-temperature relation (1175 citations)
  • Chandra Cluster Cosmology Project III: Cosmological Parameter Constraints (965 citations)

What are the main themes of his work throughout his whole career to date?

William R. Forman focuses on Astrophysics, Galaxy, Astronomy, Galaxy cluster and Elliptical galaxy. His research ties X-ray and Astrophysics together. His Galaxy and Active galactic nucleus, ROSAT, Galaxy group, Supermassive black hole and Galaxy formation and evolution investigations all form part of his Galaxy research activities.

His study brings together the fields of X-ray astronomy and Astronomy. His Galaxy cluster research includes elements of Radius, Cooling flow and Velocity dispersion. His is doing research in Virgo Cluster and Lenticular galaxy, both of which are found in Elliptical galaxy.

He most often published in these fields:

  • Astrophysics (90.88%)
  • Galaxy (46.64%)
  • Astronomy (37.18%)

What were the highlights of his more recent work (between 2016-2021)?

  • Astrophysics (90.88%)
  • Galaxy cluster (29.95%)
  • Galaxy (46.64%)

In recent papers he was focusing on the following fields of study:

His primary areas of investigation include Astrophysics, Galaxy cluster, Galaxy, Redshift and Intracluster medium. His studies in Astrophysics integrate themes in fields like X-ray and Radius. His Galaxy cluster research is within the category of Astronomy.

The concepts of his Redshift study are interwoven with issues in Cosmology, Quasar and Photon. His work in Surface brightness addresses issues such as Spectral index, which are connected to fields such as Halo and LOFAR. The various areas that William R. Forman examines in his Active galactic nucleus study include Supermassive black hole, Cooling flow and Sky.

Between 2016 and 2021, his most popular works were:

  • The case for electron re-acceleration at galaxy cluster shocks (125 citations)
  • The Case for Electron Re-Acceleration at Galaxy Cluster Shocks (122 citations)
  • Cluster Cosmology Constraints from the 2500 deg2 SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope (117 citations)

In his most recent research, the most cited papers focused on:

  • Astronomy
  • Astrophysics
  • Galaxy

His primary scientific interests are in Astrophysics, Galaxy cluster, Galaxy, Intracluster medium and Redshift. His studies link Radius with Astrophysics. His research in Radius intersects with topics in X-ray, Luminosity, Emissivity and Core.

His work carried out in the field of Galaxy cluster brings together such families of science as Shock wave, Bow shock and Planck. His Intracluster medium research entails a greater understanding of Astronomy. His study in Redshift is interdisciplinary in nature, drawing from both Cosmology and Quasar.

Best Publications

  • Chandra sample of nearby relaxed galaxy clusters: mass, gas fraction, and mass-temperature relation

    A. Vikhlinin;A. Kravtsov;W. Forman;C. Jones

  • Erratum: "Chandra Sample of Nearby Relaxed Galaxy Clusters: Mass, Gas Fraction, and Mass-Temperature Relation"

    A. Vikhlinin;A. Kravtsov;W. Forman;C. Jones

  • Chandra Cluster Cosmology Project III: Cosmological Parameter Constraints

    A. Vikhlinin;A. V. Kravtsov;R. A. Burenin;H. Ebeling

  • The Einstein /HEAO 2/ X-ray Observatory

    R. Giacconi;G. Branduardi;U. Briel;A. Epstein

  • Direct Constraints on the Dark Matter Self-Interaction Cross Section from the Merging Galaxy Cluster 1E 0657–56

    M. Markevitch;A. H. Gonzalez;D. Clowe;D. Clowe;A. Vikhlinin;A. Vikhlinin

  • A Textbook Example of a Bow Shock in the Merging Galaxy Cluster 1E0657-56

    M. Markevitch;A. H. Gonzalez;L. David;A. Vikhlinin

  • The fourth Uhuru catalog of X-ray sources.

    W. Forman;C. Jones;L. Cominsky;P. Julien

  • Chandra X-Ray Observations of the Hydra A Cluster: An Interaction between the Radio Source and the X-Ray-emitting Gas

    B. R. McNamara;M. Wise;P. E. J. Nulsen;P. E. J. Nulsen;L. P. David

  • Evolution of buoyant bubbles in M87

    E. Churazov;E. Churazov;M. Brüggen;M. Brüggen;C. R. Kaiser;H. Böhringer

  • Chandra Cluster Cosmology Project. II. Samples and X-Ray Data Reduction

    A. Vikhlinin;R. A. Burenin;H. Ebeling;W. R. Forman

  • The structure of clusters of galaxies observed with Einstein

    C. Jones;W. Forman

  • A Textbook Example of a Bow Shock in the Merging Galaxy Cluster 1E 0657–56

    M. Markevitch;A. H. Gonzalez;L. David;A. Vikhlinin

  • Galaxy clusters discovered via the Sunyaev-Zel'dovich effect in the 2500-square-degree SPT-SZ survey

    L. E. Bleem;L. E. Bleem;Brian A Stalder;T. de Haan;K. A. Aird

  • Chandra Observation of Abell 2142: Survival of Dense Subcluster Cores in a Merger

    M. Markevitch;T. J. Ponman;P. E. J. Nulsen;M. W. Bautz

  • CHANDRA STUDIES OF THE X-RAY GAS PROPERTIES OF GALAXY GROUPS

    M. Sun;G. M. Voit;M. Donahue;C. Jones

  • The Temperature Structure of 30 Nearby Clusters Observed with ASCA: Similarity of Temperature Profiles

    Maxim Markevitch;Maxim Markevitch;William R. Forman;Craig L. Sarazin;Alexey Vikhlinin;Alexey Vikhlinin

  • A catalog of intracluster gas temperatures

    L. P. David;A. Slyz;C. Jones;W. Forman

  • Chandra Temperature Profiles for a Sample of Nearby Relaxed Galaxy Clusters

    A. Vikhlinin;M. Markevitch;S. S. Murray;C. Jones

  • Host Galaxies, Clustering, Eddington Ratios, and Evolution of Radio, X-Ray, and Infrared-selected AGNs.

    Ryan C. Hickox;Christine Jones;William R. Forman;Stephen S. Murray

  • An investigation of cooling flows and general cluster properties from an X-ray image deprojection analysis of 207 clusters of galaxies

    D. A. White;C. Jones;W. Forman

Frequent Co-Authors

C. Jones
C. Jones Harvard University
Paul Nulsen
Paul Nulsen Harvard University
Alexey Vikhlinin
Alexey Vikhlinin Harvard University
Martin J. Hardcastle
Martin J. Hardcastle University of Hertfordshire
E. Churazov
E. Churazov Max Planck Society
Adrian T. Lee
Adrian T. Lee University of California, Berkeley
Ryan C. Hickox
Ryan C. Hickox Dartmouth College
Maxim Markevitch
Maxim Markevitch Harvard-Smithsonian Center for Astrophysics
John E. Carlstrom
John E. Carlstrom University of Chicago
C. L. Chang
C. L. Chang Argonne National Laboratory

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