Radiation-driven Implosion

Radiation-Driven Implosion is a theoretical astrophysical mechanism within the study of triggered star formation in which the compression and subsequent collapse of a molecular cloud or pre-stellar core are initiated by the intense ionizing radiation and associated shock fronts from a nearby massive star, distinguishing it from other star formation triggers by its reliance on radiative feedback as the primary impelling force.

217

Publications

12.1K

Citations

1.2K

Authors

216

Institutions

Publications per year

2017–2026

44

Variants

Rdi

Authors

1.2K

  1. OL
    O. L. Landen

    Lawrence Livermore National Laboratory, United States

    18 publications · 1K citations

    16

    h-index

  2. SW
    S. W. Haan

    Lawrence Livermore National Laboratory, United States

    13 publications · 863 citations

    12

    h-index

  3. AN
    A. Nikroo

    General Atomics (United States), United States

    13 publications · 582 citations

    12

    h-index

  4. DS
    D. S. Clark

    Lawrence Livermore National Laboratory, United States

    11 publications · 558 citations

    11

    h-index

  5. TD
    T. Döppner

    Lawrence Livermore National Laboratory, United States

    11 publications · 569 citations

    11

    h-index

1–5 of 1.2K

Venues

  1. Physics of Plasmas

    64 publications · 4.9K citations

    29

    h-index

  2. Physical Review Letters

    PRL · 19 publications · 1.4K citations

    18

    h-index

  3. The Astrophysical Journal

    ApJ · 17 publications · 1.5K citations

    15

    h-index

  4. 11

    h-index

  5. IEEE Transactions on Plasma Science

    11 publications · 232 citations

    10

    h-index

1–5