Planet population synthesis: The role of stellar encounters
Depending on the stellar densities, protoplanetary discs in stellar clusters undergo: background heating; disc truncation-driven by stellar encounter; and photoevaporation. Disc truncation leads to reduced characteristic sizes and disc masses that eventually halt gas giant planet formation. We inves...
Main Authors: | , , |
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Format: | Article |
Language: | English |
Published: |
Oxford University Press
2022
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Subjects: | |
Online Access: | View Fulltext in Publisher |