3D CMZ. V. A New Orbital Model of Our Galaxy’s Center, Informed by Data Across the Electromagnetic Spectrum

The 3D structure of the Milky Way’s central molecular zone (CMZ) informs our understanding of star formation cycles, black hole accretion, and the evolution of galactic nuclei. However, a comprehensive 3D model has remained elusive, as no singular data set nor theory contains the requisite informati...

Täydet tiedot

Bibliografiset tiedot

Päätekijät:	Dani R. Lipman, Cara Battersby, Daniel Walker, Maïca Clavel, B.L. DuBois, Adam Ginsburg, Jonathan D. Henshaw, Ralf S. Klessen, Elisabeth A.C. Mills, Francisco Nogueras-Lara, Mattia C. Sormani, Robin G. Tress
Aineistotyyppi:	Artigo
Kieli:	Inglês
Julkaistu:	IOP Publishing 2026-01-01
Sarja:	The Astrophysical Journal
Aiheet:	Galactic center Galaxy dynamics Milky Way Galaxy
Linkit:	https://doi.org/10.3847/1538-4357/ae561f
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