3D CMZ. IV. Distinguishing Near versus Far Distances in the Galactic Center Using Spitzer and Herschel

A comprehensive 3D model of the central 300 pc of the Milky Way, the Central Molecular Zone (CMZ) is of fundamental importance in understanding energy cycles in galactic nuclei, since the 3D structure influences the location and intensity of star formation, feedback, and black hole accretion. Curren...

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Dettagli Bibliografici

Autori principali:	Dani Lipman, Cara Battersby, Daniel L. Walker, Mattia C. Sormani, John Bally, Ashley Barnes, Adam Ginsburg, Simon C. O. Glover, Jonathan D. Henshaw, H Perry Hatchfield, Katharina Immer, Ralf S. Klessen, Steven N. Longmore, Elisabeth A. C. Mills, Rowan Smith, R. G. Tress, Danya Alboslani, Qizhou Zhang
Natura:	Artigo
Lingua:	Inglês
Pubblicazione:	IOP Publishing 2025-01-01
Serie:	The Astrophysical Journal
Soggetti:	Infrared dark clouds Interstellar dust extinction Galactic center
Accesso online:	https://doi.org/10.3847/1538-4357/adb5ee
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