Pulsar Populations

Pulsar Populations is a scientific construct in astrophysics that denotes the collective distribution and statistical properties of pulsars within globular clusters, distinguished from field pulsar populations by their dynamical formation channels, cluster-centric spatial distribution, and enhanced incidence of binary systems due to dense stellar environments.

683

Publications

49.1K

Citations

3.3K

Authors

739

Institutions

Publications per year

2017–2026

110

Authors

3.3K

  1. RN
    R. N. Manchester

    Commonwealth Scientific and Industrial Research Organisation, Australia

    35 publications · 5.2K citations

    29

    h-index

  2. AG
    A. G. Lyne

    University of Manchester, United Kingdom

    32 publications · 4.8K citations

    29

    h-index

  3. DR
    D. R. Lorimer

    West Virginia University, United States

    37 publications · 6.6K citations

    29

    h-index

  4. MK
    M. Krämer

    University of Manchester, United Kingdom

    29 publications · 2.8K citations

    21

    h-index

  5. SM
    S. M. Ransom

    National Radio Astronomy Observatory, United States

    23 publications · 3.9K citations

    20

    h-index

1–5 of 3.3K

Venues

  1. The Astrophysical Journal

    ApJ · 130 publications · 11.4K citations

    58

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    121 publications · 8.4K citations

    48

    h-index

  3. Nature

    99 publications · 8.7K citations

    43

    h-index

  4. Astronomy and Astrophysics

    49 publications · 2.8K citations

    30

    h-index

  5. The Astronomical Journal

    AJ · 14 publications · 689 citations

    14

    h-index

1–5