Global and Local Infall in the ASHES Sample (GLASHES). III. Physical Parameters of Contracting Motion onto Dense Cores in 70 mu m Dark Massive Clumps

arXiv:2610.10676 · astro-ph.GA, astro-ph.SR · Submitted 2026-10-07 · Read on arXiv

astro-ph.GA, astro-ph.SR

Submitted: 2026-10-07

Updated: 2026-10-07

Terminology

• Core — 261× in this paper · explained in 2 episodes
• Velocity Dispersion — 14× in this paper · explained in 2 episodes
• Adam — 2× in this paper · explained in 2 episodes
• Degeneracy — 2× in this paper · explained in 3 episodes
• Markov Chain Monte Carlo — 2× in this paper
• Anti-correlation — 1× in this paper · explained in 3 episodes
• Benchmark — 1× in this paper · explained in 2 episodes
• Calibration — 1× in this paper · explained in 7 episodes
• Consistency — 1× in this paper · explained in 3 episodes
• Cooperation — 1× in this paper · explained in 2 episodes
• Stellar Feedback — 1× in this paper · explained in 2 episodes
• Total Power — 1× in this paper
• Trace — 1× in this paper · explained in 2 episodes

Sources

• Studying Infall
• Challenges in probing turbulent and magnetic support in cores: the W43-MM1 protocluster case study
• Dynamical Accretion Flows -- ALMAGAL: Flows along filamentary structures in high-mass star-forming clusters
• Evolution of starless cores in massive clumps seen by the ALMA ASHES and QUARKS surveys

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