Bartkiewicz, Anna; Burns, Ross; Olech, Mateusz; Durjasz, Michał; Uno, Yuri; Sakai, Nobuyuki; [i in.]
(2023)
High-mass protostars (M⋆ > 8M⊙) are thought to gain the majority of their mass via short, intense bursts of growth. This episodic accretion is thought to be facilitated by gravitationally unstable and subsequently inhomogeneous ...