Galactic Dust Distribution

Galactic Dust Distribution is a spatial model in interstellar astronomy that characterizes the three-dimensional arrangement of dust particles in the Milky Way galaxy, distinguishing it from other extinction components by specifying the density, composition, and location of dust as a function of galactic coordinates.

163

Publications

12.9K

Citations

633

Authors

305

Institutions

Publications per year

2017–2026

38

Authors

633

  1. SB
    S. Bianchi

    Arcetri Astrophysical Observatory, Italy

    7 publications · 365 citations

    7

    h-index

  2. MS
    M. Schartmann

    Max Planck Institute for Extraterrestrial Physics, Germany

    6 publications · 610 citations

    6

    h-index

  3. JF
    J. Fritz

    Osservatorio Astronomico di Padova, Italy

    5 publications · 758 citations

    5

    h-index

  4. MB
    M. Baes

    Ghent University, Belgium

    4 publications · 566 citations

    4

    h-index

  5. EM
    E. M. Xilouris

    National Observatory of Athens, Greece

    4 publications · 274 citations

    4

    h-index

1–5 of 633

Venues

  1. The Astrophysical Journal

    ApJ · 41 publications · 3.3K citations

    28

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    36 publications · 3.1K citations

    26

    h-index

  3. Astronomy and Astrophysics

    27 publications · 3.3K citations

    22

    h-index

  4. The Astronomical Journal

    AJ · 9 publications · 521 citations

    9

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 5 publications · 331 citations

    5

    h-index

1–5