Dust Emissivity

Dust Emissivity is a physical property that quantifies the efficiency with which interstellar dust grains emit electromagnetic radiation per unit mass at a given wavelength, distinguishing it from other emission processes by its dependence on grain composition, size distribution, and temperature.

287

Publications

20.6K

Citations

1.5K

Authors

526

Institutions

Publications per year

2017–2026

62

Authors

1.5K

  1. MJ
    M. Juvela

    University of Helsinki, Finland

    16 publications · 1.1K citations

    15

    h-index

  2. RP
    R. Paladini

    California Institute of Technology, United States

    13 publications · 1.1K citations

    13

    h-index

  3. MB
    M. Baes

    Ghent University, Belgium

    12 publications · 1.1K citations

    12

    h-index

  4. JB
    J.-P. Bernard

    Centre National de la Recherche Scientifique, France

    12 publications · 1K citations

    12

    h-index

  5. PG
    P. G. Martin

    University of Toronto, Canada

    12 publications · 742 citations

    12

    h-index

1–5 of 1.5K

Venues

  1. The Astrophysical Journal

    ApJ · 74 publications · 7.4K citations

    42

    h-index

  2. Astronomy and Astrophysics

    58 publications · 4.7K citations

    38

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    37 publications · 2.1K citations

    26

    h-index

  4. The Astronomical Journal

    AJ · 8 publications · 178 citations

    8

    h-index

  5. Solar Energy

    5 publications · 257 citations

    5

    h-index

1–5