The ALMaQUEST Survey. XIII. Understanding Radial Trends in Star Formation Quenching via the Relative Roles of Gas Availability and Star Formation Efficiency

Star formation quenching is one of the key processes that shape the evolution of galaxies. In this study, we investigate the changes in molecular gas and star formation properties as galaxies transit from the star-forming main sequence to the passive regime. Our analysis reveals that as galaxies mov...

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Veröffentlicht in:	The Astrophysical journal Jg. 964; H. 2; S. 120 - 141
Hauptverfasser:	Pan, Hsi-An, Lin, Lihwai, Ellison, Sara L., Thorp, Mallory D., Sánchez, Sebastián F., Bluck, Asa F. L., Belfiore, Francesco, Piotrowska, Joanna M., Scudder, Jillian M., Baker, William M.
Format:	Journal Article
Sprache:	Englisch
Veröffentlicht:	Philadelphia The American Astronomical Society 01.04.2024 IOP Publishing
Schlagworte:	Galactic evolution Galaxies Galaxy evolution Interstellar medium Molecular gases Quenching Star & galaxy formation Star formation Star formation rate Stars Stars & galaxies
ISSN:	0004-637X, 1538-4357
Online-Zugang:	Volltext
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