Challenges in probing turbulent and magnetic support in cores: the W43-MM1 protocluster case study

arXiv:2607.10029 · astro-ph.GA · Submitted 2026-07-10 · Read on arXiv

M. Valeille-Manet, F. Louvet, F. Motte, A. M. Stutz, C. Arce-Tord, P. C. Cortés, M. Fernandez-Lopez, N. A. Sandoval-Garrido, P. Sanhueza, R. H. Álvarez-Gutiérrez, S. Chevalier, A. Ginsburg, A. Koley, P. Saha, S. Savorgnano, R. Veyry

astro-ph.GA

Submitted: 2026-07-10

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Core — 353× in this paper · explained in 2 episodes
• Velocity Dispersion — 65× in this paper · explained in 2 episodes
• Trace — 8× in this paper · explained in 2 episodes
• Consistency — 2× in this paper · explained in 3 episodes
• Alignment — 1× in this paper · explained in 1 episode
• Ambipolar Diffusion — 1× in this paper · explained in 1 episode
• Anti-correlation — 1× in this paper · explained in 3 episodes
• Cooperation — 1× in this paper · explained in 2 episodes
• Japan Society for the Promotion of Science — 1× in this paper
• Signal-to-noise ratio (SNR) — 1× in this paper · explained in 2 episodes
• Stellar Feedback — 1× in this paper · explained in 2 episodes
• alpha — 1× in this paper · explained in 1 episode

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