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What is G323.46-0.08 Accretion Outburst Analysis about?

This study investigates the role of thermal instability in episodic accretion bursts in high-mass star formation using a two-dimensional hydrodynamical model. The findings reveal that thermal instability significantly alters disk structure and leads to observable outbursts, although these events are not bright enough to match some rapid observed phenomena. The results suggest that while thermal instability is influential, additional mechanisms are necessary to fully explain the diversity of outburst behavio

Author

Omar López Rubio

Language

EN