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...

詳細記述

書誌詳細
主要な著者: Francesca Perrotta, Martina Torsello, Marika Giulietti, Andrea Lapi
フォーマット: 論文
言語:English
出版事項: MDPI AG 2024-04-01
シリーズ:Galaxies
主題:
オンライン・アクセス:https://www.mdpi.com/2075-4434/12/2/18