Simple Stellar Populations

Simple Stellar Populations is a theoretical astrophysical model representing a coeval, chemically homogeneous group of stars formed at the same time and location, distinguished by its assumption of negligible spread in age and metallicity, used to study the collective evolution of stars within a single stellar generation.

374

Publications

29.8K

Citations

1.1K

Authors

436

Institutions

Publications per year

2017–2026

65

Variants

Ssps

Authors

1.1K

  1. NB
    N. Bastian

    Liverpool John Moores University, United Kingdom

    16 publications · 1.2K citations

    15

    h-index

  2. SS
    S. S. Larsen

    Radboud University Nijmegen, Netherlands

    11 publications · 452 citations

    11

    h-index

  3. AB
    A. Bressan

    Osservatorio Astronomico di Padova, Italy

    9 publications · 1.5K citations

    9

    h-index

  4. JP
    Jean P. Brodie

    University of California, Santa Cruz, United States

    9 publications · 693 citations

    9

    h-index

  5. AP
    A. P. Milone

    Osservatorio Astronomico di Padova, Italy

    9 publications · 721 citations

    9

    h-index

1–5 of 1.1K

Venues

  1. 44

    h-index

  2. The Astrophysical Journal

    ApJ · 75 publications · 7.2K citations

    38

    h-index

  3. Astronomy and Astrophysics

    54 publications · 4.3K citations

    31

    h-index

  4. The Astronomical Journal

    AJ · 31 publications · 2.1K citations

    23

    h-index

  5. The Astrophysical Journal Letters

    13 publications · 978 citations

    13

    h-index

1–5