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Can Clump Properties Predict Core Distribution in Star Formation? A Statistical Analysis of MHD Simulations

Fuente: arXiv

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Détails bibliographiques
Auteurs principaux:	Chen, Wei-An, Clarke, Seamus D., Tang, Ya-Wen
Format:	Preprint
Publié:	2025
Sujets:	Astrophysics of Galaxies
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

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