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Nuclear spirals in the inner Milky Way

We use hydrodynamical simulations to construct a new coherent picture for the gas flow in the Central Molecular Zone (CMZ), the region of our Galaxy within R ≲ 500  pc. We relate connected structures observed in (l, b, v) data cubes of molecular tracers to nuclear spiral arms. These arise naturally...

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Hauptverfasser: Ridley, Matthew G.L. (VerfasserIn) , Sormani, Mattia C. (VerfasserIn) , Treß, Robin G. (VerfasserIn) , Klessen, Ralf S. (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 21 April 2017
In: Monthly notices of the Royal Astronomical Society
Year: 2017, Jahrgang: 469, Heft: 2, Pages: 2251-2262
ISSN:1365-2966
DOI:10.1093/mnras/stx944
Online-Zugang:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stx944
Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/469/2/2251/3747502/Nuclear-spirals-in-the-inner-Milky-Way
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Verfasserangaben:Matthew G.L. Ridley, Mattia C. Sormani, Robin G. Treß, John Magorrian, Ralf S. Klessen

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