Theory of Turbulent Equilibrium Spheres with Power-law Linewidth–Size Relation

Dense cores inherit turbulent motions from the interstellar medium in which they form. As a tool for comparison to both simulations and observations, it is valuable to construct theoretical core models that can relate their internal density and velocity structure while predicting their stability to...

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Bibliographic Details
Main Authors: Sanghyuk Moon, Eve C. Ostriker
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad7813