Radiative Transfer Effects

Radiative Transfer Effects is a physical phenomenon in astrophysical environments representing the genus of radiative processes, differentiated by its specific influence on the propagation, absorption, and emission of electromagnetic radiation through dusty and gaseous media in star-forming regions, thereby affecting observed spectral energy distributions and molecular line intensities.

1.1K

Publications

60.6K

Citations

3.6K

Authors

1.1K

Institutions

Publications per year

2017–2026

292

Authors

3.6K

  1. SK
    S. K. Solanki

    Max Planck Institute for Solar System Research, Germany

    11 publications · 323 citations

    11

    h-index

  2. LH
    Lars Hernquist

    Center for Astrophysics Harvard & Smithsonian, United States

    8 publications · 993 citations

    8

    h-index

  3. RH
    R. Holzreuter

    ETH Zurich, Switzerland

    8 publications · 221 citations

    8

    h-index

  4. KK
    K. Krishna Moorthy

    Vikram Sarabhai Space Centre, India

    7 publications · 467 citations

    7

    h-index

  5. AM
    Alexander Marshak

    Goddard Space Flight Center, United States

    7 publications · 744 citations

    7

    h-index

1–5 of 3.6K

Venues

  1. The Astrophysical Journal

    ApJ · 150 publications · 11.1K citations

    57

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    111 publications · 6.6K citations

    46

    h-index

  3. Journal of Geophysical Research Atmospheres

    JGR · 71 publications · 6.8K citations

    42

    h-index

  4. Astronomy and Astrophysics

    93 publications · 4.4K citations

    38

    h-index

  5. Atmospheric chemistry and physics

    41 publications · 2.7K citations

    29

    h-index

1–5