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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| 主要な著者: | , , , |
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| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
MDPI AG
2024-04-01
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| 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 |
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