VVV-WIT-13: An eruptive young star with cool molecular features
Date Issued
2025-11
Author(s) USM
Montesinos, Matías
DOI
10.1051/0004-6361/202556048
Abstract
Context. Outburst phenomena are observed at different stages of stellar evolution, due to the enhancement of the mass accretion rate on protostars or even stellar merger events. In the case of a young stellar object (YSO), the episodic mass accretion even
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