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Cooling process of the high-mass young stellar object G24.33+0.14 following an accretion burst

Fuente: arXiv

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Détails bibliographiques
Auteurs principaux:	Xu, Xiaoyun, Chen, Xi, Yang, Yang
Format:	Preprint
Publié:	2025
Sujets:	Astrophysics of Galaxies Solar and Stellar Astrophysics
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

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