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

Fuente: arXiv

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Bibliographic Details
Main Authors:	Xu, Xiaoyun, Chen, Xi, Yang, Yang
Format:	Preprint
Published:	2025
Subjects:	Astrophysics of Galaxies Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2504.19782