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
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| Main Authors: | , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
2019 January 7
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2019, Volume: 484, Issue: 1, Pages: 1213-1219 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stz046 |
| Online Access: | Verlag, Volltext: http://dx.doi.org/10.1093/mnras/stz046 Verlag, Volltext: https://academic.oup.com/mnras/article/484/1/1213/5280055 
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| Author Notes: | Mattia C. Sormani and Ashley T. Barnes |
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Mass inflow rate into the Central Molecular Zone: observational determination and evidence of episodic accretion
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