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3D CMZ. I. Central Molecular Zone Overview

The Central Molecular Zone (CMZ) is the largest reservoir of dense molecular gas in the Galaxy and is heavily obscured in the optical and near-IR. We present an overview of the far-IR dust continuum, where the molecular clouds are revealed, provided by Herschel in the inner 40° (∣ l ∣ < 20°) of the...

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Enregistré dans:
Auteurs principaux: Cara Battersby, Daniel L. Walker, Ashley Barnes, Adam Ginsburg, Dani Lipman, Danya Alboslani, H Perry Hatchfield, John Bally, Simon C. O. Glover, Jonathan D. Henshaw, Katharina Immer, Ralf S. Klessen, Steven N. Longmore, Elisabeth A. C. Mills, Sergio Molinari, Rowan Smith, Mattia C. Sormani, Robin G. Tress, Qizhou Zhang
Format: Artigo
Langue:Inglês
Publié: IOP Publishing 2025-01-01
Collection:The Astrophysical Journal
Sujets:
Galactic center
Star formation
Dust continuum emission
Far infrared astronomy
Accès en ligne:https://doi.org/10.3847/1538-4357/adb5f0
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