Mass inflow rate into the Central Molecular Zone: observational determination and evidence of episodic accretion

ABSTRACT. It is well known that the Galactic bar drives a gas inflow into the Central Molecular Zone, which fuels star formation, accretion on to the central s

Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Sormani, Mattia C. (VerfasserIn) , Barnes, Ashley T. (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 2019 January 7
In: Monthly notices of the Royal Astronomical Society
Year: 2019, Jahrgang: 484, Heft: 1, Pages: 1213-1219
ISSN:1365-2966
DOI:10.1093/mnras/stz046
Online-Zugang:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/stz046
Verlag, Volltext: https://academic.oup.com/mnras/article/484/1/1213/5280055
Volltext
Verfasserangaben:Mattia C. Sormani and Ashley T. Barnes
Beschreibung
Zusammenfassung:ABSTRACT. It is well known that the Galactic bar drives a gas inflow into the Central Molecular Zone, which fuels star formation, accretion on to the central s
Beschreibung:Gesehen am 04.02.2019
Beschreibung:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stz046