A High Resolution View of Three Massive Young Stellar Objects in the Magellanic Clouds

arXiv:2609.27121 · astro-ph.GA · Submitted 2026-09-22 · Read on arXiv

astro-ph.GA

Submitted: 2026-09-22

Updated: 2026-09-22

Terminology

• Core — 42× in this paper · explained in 2 episodes
• Metallicity — 16× in this paper · explained in 3 episodes
• Trace — 11× in this paper · explained in 2 episodes
• Aperture — 7× in this paper · explained in 1 episode
• Calibration — 3× in this paper · explained in 7 episodes
• Degeneracy — 2× in this paper · explained in 3 episodes
• Minimum Spanning Tree — 2× in this paper
• Velocity Dispersion — 2× in this paper · explained in 2 episodes
• APEX — 1× in this paper · explained in 1 episode
• Abundance — 1× in this paper · explained in 1 episode
• Alignment — 1× in this paper · explained in 1 episode
• Benchmark — 1× in this paper · explained in 2 episodes
• Clustering — 1× in this paper · explained in 2 episodes
• Cooperation — 1× in this paper · explained in 2 episodes
• Forward modeling — 1× in this paper · explained in 2 episodes
• Frequency Dependence — 1× in this paper · explained in 2 episodes

Sources

• HOTDISK. Finding Massive Protostellar Disks with Water and Refractory Molecular Species

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