D-Index & Metrics Best Publications

D-Index & Metrics D-index (Discipline H-index) only includes papers and citation values for an examined discipline in contrast to General H-index which accounts for publications across all disciplines.

Discipline name D-index D-index (Discipline H-index) only includes papers and citation values for an examined discipline in contrast to General H-index which accounts for publications across all disciplines. Citations Publications World Ranking National Ranking
Physics D-index 81 Citations 55,115 218 World Ranking 2113 National Ranking 1087

Research.com Recognitions

Awards & Achievements

2020 - Member of the National Academy of Sciences

Overview

What is he best known for?

The fields of study he is best known for:

  • Galaxy
  • Astronomy
  • Milky Way

John Kormendy mainly focuses on Astrophysics, Astronomy, Galaxy, Elliptical galaxy and Bulge. His work is connected to Galaxy merger, Supermassive black hole, Lenticular galaxy, Velocity dispersion and M–sigma relation, as a part of Astrophysics. His Galaxy merger research is multidisciplinary, relying on both Galaxy group and Interacting galaxy.

Galaxy formation and evolution and Brightest cluster galaxy are among the areas of Astronomy where John Kormendy concentrates his study. His study in Galaxy is interdisciplinary in nature, drawing from both Cosmology and Black hole. His Elliptical galaxy research is multidisciplinary, incorporating perspectives in Accretion and Luminous infrared galaxy.

His most cited work include:

  • The Demography of massive dark objects in galaxy centers (3345 citations)
  • A Relationship between Nuclear Black Hole Mass and Galaxy Velocity Dispersion (3321 citations)
  • The Demography of Massive Dark Objects in Galaxy Centres (3251 citations)

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

His primary areas of investigation include Astrophysics, Galaxy, Astronomy, Bulge and Elliptical galaxy. His research related to Velocity dispersion, Supermassive black hole, Black hole, Galaxy formation and evolution and Stars might be considered part of Astrophysics. He interconnects Quasar and Active galactic nucleus in the investigation of issues within Supermassive black hole.

His Galaxy study incorporates themes from Brightness and Dark matter. His Lenticular galaxy, Luminous infrared galaxy, Galaxy merger, Hubble sequence and Interacting galaxy study are his primary interests in Astronomy. His Bulge study integrates concerns from other disciplines, such as Dust lane, Radial velocity, Milky Way, Photometry and Spiral galaxy.

He most often published in these fields:

  • Astrophysics (103.70%)
  • Galaxy (74.75%)
  • Astronomy (59.26%)

What were the highlights of his more recent work (between 2011-2020)?

  • Astrophysics (103.70%)
  • Galaxy (74.75%)
  • Bulge (40.07%)

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

John Kormendy mainly investigates Astrophysics, Galaxy, Bulge, Astronomy and Elliptical galaxy. His study in Supermassive black hole, Velocity dispersion, Galaxy formation and evolution, Black hole and Galaxy merger falls within the category of Astrophysics. In the field of Supermassive black hole, his study on Intermediate-mass black hole overlaps with subjects such as Coevolution.

The concepts of his Galaxy merger study are interwoven with issues in Lenticular galaxy and Interacting galaxy. John Kormendy usually deals with Galaxy and limits it to topics linked to Dark matter and Galaxy rotation curve. His Bulge research is multidisciplinary, relying on both Milky Way and Kinematics.

Between 2011 and 2020, his most popular works were:

  • Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies (2478 citations)
  • A REVISED PARALLEL-SEQUENCE MORPHOLOGICAL CLASSIFICATION OF GALAXIES: STRUCTURE AND FORMATION OF S0 AND SPHEROIDAL GALAXIES (295 citations)
  • The Bulge Radial Velocity Assay (BRAVA). II. Complete Sample and Data Release (231 citations)

This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.

Best Publications

The Demography of Massive Dark Objects in Galaxy Centres

John Magorrian;Scott Tremaine;Douglas Richstone;Ralf Bender.
arXiv: Astrophysics (1997)

6343 Citations

The Demography of massive dark objects in galaxy centers

John Magorrian;Scott Tremaine;Scott Tremaine;Douglas Richstone;Ralf Bender.
The Astronomical Journal (1998)

4804 Citations

A Relationship between Nuclear Black Hole Mass and Galaxy Velocity Dispersion

Karl Gebhardt;Ralf Bender;Gary Bower;Alan Dressler.
The Astrophysical Journal (2000)

4562 Citations

Inward Bound—The Search for Supermassive Black Holes in Galactic Nuclei

John Kormendy;Douglas Richstone.
Annual Review of Astronomy and Astrophysics (1995)

3186 Citations

THE SLOPE OF THE BLACK HOLE MASS VERSUS VELOCITY DISPERSION CORRELATION

Scott Tremaine;Karl Gebhardt;Ralf Bender;Gary Bower.
The Astrophysical Journal (2002)

3076 Citations

Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies

John Kormendy;Luis C. Ho.
Annual Review of Astronomy and Astrophysics (2013)

3075 Citations

The M-σ and M-L Relations in Galactic Bulges, and Determinations of Their Intrinsic Scatter

Kayhan Gültekin;Douglas D.O. Richstone;Karl Gebhardt;Tod Lauer.
The Astrophysical Journal (2009)

2288 Citations

The M-sigma and M-L Relations in Galactic Bulges and Determinations of their Intrinsic Scatter

Kayhan Gultekin;Douglas O. Richstone;Karl Gebhardt;Tod R. Lauer.
arXiv: Astrophysics of Galaxies (2009)

2214 Citations

Secular Evolution and the Formation of Pseudobulges in Disk Galaxies

John Kormendy;Robert C. Kennicutt.
Annual Review of Astronomy and Astrophysics (2004)

1955 Citations

The centers of early-type galaxies with HST. IV. Central parameter relations

S. M. Faber;Scott Tremaine;Edward A. Ajhar;Yong Ik Byun;Yong Ik Byun.
The Astronomical Journal (1997)

1138 Citations

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