Long-period Variables

Long-Period Variables is a class of pulsating variable stars characterized by orbital periods exceeding 100 days, distinguished from other variable star types by their extended periodicity and association with late spectral types undergoing radial pulsations in the asymptotic giant branch phase.

359

Publications

15.4K

Citations

918

Authors

361

Institutions

Publications per year

2017–2026

36

Variants

Lpvs

Authors

918

  1. PR
    P. R. Wood

    Australian National University, Australia

    29 publications · 1.9K citations

    22

    h-index

  2. TL
    T. Lebzelter

    University of Vienna, Austria

    15 publications · 545 citations

    13

    h-index

  3. MW
    M. W. Feast

    South African Radio Astronomy Observatory, South Africa

    9 publications · 580 citations

    9

    h-index

  4. MS
    M. S. Bessell

    Australian National University, Australia

    8 publications · 587 citations

    8

    h-index

  5. MT
    Michele Trabucchi

    Osservatorio Astronomico di Padova, Italy

    7 publications · 310 citations

    7

    h-index

1–5 of 918

Venues

  1. The Astrophysical Journal

    ApJ · 106 publications · 4.5K citations

    37

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    68 publications · 2.9K citations

    30

    h-index

  3. The Astronomical Journal

    AJ · 45 publications · 2.1K citations

    29

    h-index

  4. Astronomy and Astrophysics

    46 publications · 1.9K citations

    26

    h-index

  5. The Astrophysical Journal Supplement Series

    13 publications · 744 citations

    13

    h-index

1–5