Pulsar Spin-down

Pulsar Spin-Down is the gradual decrease in the rotation rate of a pulsar over time, arising from the loss of rotational energy primarily through magnetic dipole radiation, relativistic particle winds, and gravitational wave emission.

414

Publications

28.6K

Citations

3.9K

Authors

699

Institutions

Publications per year

2017–2026

102

Authors

3.9K

  1. AG
    A. G. Lyne

    University of Manchester, United Kingdom

    18 publications · 3K citations

    18

    h-index

  2. SJ
    S. Johnston

    Commonwealth Scientific and Industrial Research Organisation, Australia

    18 publications · 1.1K citations

    17

    h-index

  3. PW
    P. Weltevrede

    University of Manchester, United Kingdom

    16 publications · 1.3K citations

    16

    h-index

  4. BW
    B. W. Stappers

    University of Manchester, United Kingdom

    16 publications · 2.3K citations

    16

    h-index

  5. RN
    R. N. Manchester

    Commonwealth Scientific and Industrial Research Organisation, Australia

    12 publications · 1.2K citations

    13

    h-index

1–5 of 3.9K

Venues

  1. The Astrophysical Journal

    ApJ · 139 publications · 11.5K citations

    59

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    100 publications · 5.6K citations

    43

    h-index

  3. Astronomy and Astrophysics

    24 publications · 866 citations

    19

    h-index

  4. The Astrophysical Journal Letters

    15 publications · 730 citations

    15

    h-index

  5. Nature

    16 publications · 2.9K citations

    14

    h-index

1–5