Molecules in the shadows of the protoplanetary disk HD 143006: Evidence for C/O 1 from simultaneously modeling fourteen ALMA lines

arXiv:2609.26433 · astro-ph.EP · Submitted 2026-09-22 · Read on arXiv

astro-ph.EP

Submitted: 2026-09-22

Updated: 2026-09-22

Comments: A&A accepted; version prior to language editing. 32 pages, 21 figures

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

Terminology

• Abundance — 32× in this paper · explained in 1 episode
• Calibration — 8× in this paper · explained in 7 episodes
• Spectral Energy Distribution — 5× in this paper
• Trace — 2× in this paper · explained in 2 episodes
• Accuracy — 1× in this paper · explained in 1 episode
• Consistency — 1× in this paper · explained in 3 episodes
• Cooperation — 1× in this paper · explained in 2 episodes

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