Models of rotating coronae

Fitting equilibrium dynamical models to observational data is an essential step in understanding the structure of the gaseous hot haloes that surroun

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Hauptverfasser: Sormani, Mattia C. (VerfasserIn) , Klessen, Ralf S. (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 2018 September 14
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 481, Heft: 3, Pages: 3370-3381
ISSN:1365-2966
DOI:10.1093/mnras/sty2500
Online-Zugang:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty2500
Verlag, Volltext: https://academic.oup.com/mnras/article/481/3/3370/5097896
Volltext
Verfasserangaben:Mattia C. Sormani, Emanuele Sobacchi, Gabriele Pezzulli, James Binney and Ralf S. Klessen

MARC

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