Protoplanetary Disk Spectroscopy

Protoplanetary Disk Spectroscopy is a specialized observational method in spectral line astronomy that analyzes the electromagnetic radiation emitted or absorbed by molecular and atomic species within circumstellar disks around young stars to infer physical and chemical conditions during planet formation.

532

Publications

43.3K

Citations

1.7K

Authors

556

Institutions

Publications per year

2017–2026

238

Authors

1.7K

  1. EF
    E. F. van Dishoeck

    Leiden University, Netherlands

    53 publications · 5K citations

    39

    h-index

  2. SM
    Sean M. Andrews

    Center for Astrophysics Harvard & Smithsonian, United States

    41 publications · 5.1K citations

    34

    h-index

  3. KI
    Karin I. Öberg

    Center for Astrophysics Harvard & Smithsonian, United States

    36 publications · 4.7K citations

    31

    h-index

  4. DJ
    David J. Wilner

    Center for Astrophysics Harvard & Smithsonian, United States

    31 publications · 4.6K citations

    27

    h-index

  5. EA
    Edwin A. Bergin

    University of Michigan, United States

    29 publications · 2.9K citations

    27

    h-index

1–5 of 1.7K

Venues

  1. The Astrophysical Journal

    ApJ · 139 publications · 10.6K citations

    58

    h-index

  2. Astronomy and Astrophysics

    142 publications · 9K citations

    56

    h-index

  3. The Astrophysical Journal Letters

    47 publications · 4.6K citations

    34

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    25 publications · 1.5K citations

    19

    h-index

  5. The Astronomical Journal

    AJ · 22 publications · 1.5K citations

    18

    h-index

1–5