Astrochemistry of the Molecular Gas in Dusty Star-Forming Galaxies at the Cosmic Noon

Far-infrared and submillimeter observations have established the fundamental role of dust-obscured star formation in the assembly of stellar mass over the past ∼12 billion years. At z = 2–4, the so-called “cosmic noon”, the bulk of star formation is enshrouded in dust, and dusty star-forming galaxie...

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Bibliographic Details
Main Authors: Francesca Perrotta, Martina Torsello, Marika Giulietti, Andrea Lapi
Format: Article
Language:English
Published: MDPI AG 2024-04-01
Series:Galaxies
Subjects:
Online Access:https://www.mdpi.com/2075-4434/12/2/18