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
Parents
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1–5 of 217
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Lawrence Livermore National Laboratory
Livermore, United States
30 h-index
630 publications
37.5K citations

University of Rochester
Rochester, United States
21 h-index
244 publications
8K citations
Los Alamos National Laboratory
Los Alamos, United States
20 h-index
208 publications
8K citations
Energetics (United States)
Columbia, United States
17 h-index
190 publications
6K citations
Sandia National Laboratories
Albuquerque, United States
17 h-index
167 publications
8.2K citations
General Atomics (United States)
San Diego, United States
15 h-index
124 publications
3.9K citations

United States Naval Research Laboratory
Washington, United States
15 h-index
76 publications
2.4K citations
The University of Osaka
Osaka, Japan
14 h-index
127 publications
7.8K citations
1–8 of 216
64 publications · 4.9K citations
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PRL · 19 publications · 1.4K citations
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ApJ · 17 publications · 1.5K citations
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12 publications · 633 citations
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11 publications · 232 citations
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