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Line profiles of cores within clusters: III. What is the most reliable tracer of core collapse in dense clusters?

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Weitere Verfasser: Chira, Roxana-Adela (BerichterstatterIn) , Smith, Rowan J. (BerichterstatterIn) , Klessen, Ralf S. (BerichterstatterIn) , Shetty, Rahul (BerichterstatterIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 2014
In: Monthly notices of the Royal Astronomical Society
Year: 2014, Jahrgang: 444, Heft: 1, Pages: 874-886
ISSN:1365-2966
DOI:10.1093/mnras/stu1497
Online-Zugang:Verlag, kostenfrei, Volltext: http://mnras.oxfordjournals.org/content/444/1/874
Resolving-System, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stu1497
Volltext
Verfasserangaben:Roxana-Adela Chira; Rowan J. Smith; Ralf S. Klessen ... Rahul Shetty

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