Open Cluster Spectroscopy

Open Cluster Spectroscopy is a spectroscopic method that systematically analyzes the collective spectral characteristics of stars within open clusters to determine their physical properties, chemical compositions, and evolutionary states, distinguishing it from broader stellar spectroscopy by its focused application to coeval, gravitationally unbound stellar populations.

441

Publications

21.8K

Citations

1.1K

Authors

445

Institutions

Publications per year

2017–2026

79

Authors

1.1K

  1. AB
    A. Bragaglia

    Osservatorio Astronomico di Padova, Italy

    28 publications · 1.4K citations

    21

    h-index

  2. GC
    G. Carraro

    Osservatorio Astronomico di Padova, Italy

    24 publications · 1.3K citations

    20

    h-index

  3. LM
    L. Magrini

    Arcetri Astrophysical Observatory, Italy

    18 publications · 1K citations

    17

    h-index

  4. SR
    S. Randich

    Arcetri Astrophysical Observatory, Italy

    18 publications · 1.5K citations

    16

    h-index

  5. VD
    V. D’Orazi

    Osservatorio Astronomico di Padova, Italy

    15 publications · 805 citations

    15

    h-index

1–5 of 1.1K

Venues

  1. Astronomy and Astrophysics

    120 publications · 5.9K citations

    47

    h-index

  2. The Astronomical Journal

    AJ · 76 publications · 4.4K citations

    38

    h-index

  3. The Astrophysical Journal

    ApJ · 64 publications · 3.9K citations

    32

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    65 publications · 2.4K citations

    27

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 16 publications · 546 citations

    14

    h-index

1–5