The fragmentation of molecular clouds in starburst environments

A significant amount of star formation occurs and has occurred in environments unlike the solar neighbourhood. The majority of stars formed closer to the peak of the cosmic star formation rate

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Bibliographic Details
Main Authors: Cusack, Matt T. (Author) , Clark, Paul C. (Author) , Glover, Simon (Author) , Klessen, Ralf S. (Author) , Girichidis, Philipp (Author) , Whitworth, Anthony P. (Author) , Priestley, Felix (Author)
Format: Article (Journal)
Language:English
Published: February 2025
In: Monthly notices of the Royal Astronomical Society
Year: 2025, Volume: 536, Issue: 4, Pages: 3518-3536
ISSN:1365-2966
DOI:10.1093/mnras/stae2812
Online Access:Verlag, kostenfrei, Volltext: https://doi.org/10.1093/mnras/stae2812
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Author Notes:Matt T. Cusack, Paul C. Clark, Simon C.O. Glover, Ralf S. Klessen, Philipp Girichidis, Anthony P. Whitworth and Felix D. Priestley
Description
Summary:A significant amount of star formation occurs and has occurred in environments unlike the solar neighbourhood. The majority of stars formed closer to the peak of the cosmic star formation rate
Item Description:Gesehen am 22.10.2025
Veröffentlicht am 23. Dezember 2024
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stae2812