Silicate Emission Features

Silicate Emission Features is a spectral signature characterized by distinct infrared emission bands arising from vibrational modes of silicate minerals in astrophysical environments, distinguishing it from other dust emission components by its specific wavelength diagnostics associated with silica-based molecular structures.

611

Publications

36.5K

Citations

1.6K

Authors

545

Institutions

Publications per year

2017–2026

51

Authors

1.6K

  1. DM
    D. M. Watson

    University of Rochester, United States

    21 publications · 1.8K citations

    18

    h-index

  2. JB
    J. Bouwman

    Max Planck Institute for Astronomy, Germany

    18 publications · 1.4K citations

    16

    h-index

  3. LB
    L. B. F. M. Waters

    University of Amsterdam, Netherlands

    17 publications · 1.4K citations

    15

    h-index

  4. PF
    P. F. Roche

    University of Oxford, United Kingdom

    20 publications · 756 citations

    15

    h-index

  5. WJ
    W. J. Forrest

    University of Rochester, United States

    17 publications · 1.3K citations

    15

    h-index

1–5 of 1.6K

Venues

  1. The Astrophysical Journal

    ApJ · 211 publications · 14.4K citations

    70

    h-index

  2. Astronomy and Astrophysics

    68 publications · 4.8K citations

    41

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    64 publications · 3.2K citations

    29

    h-index

  4. The Astronomical Journal

    AJ · 28 publications · 1.3K citations

    22

    h-index

  5. Icarus

    14 publications · 735 citations

    14

    h-index

1–5