Interferometric molecular line observations toward the 21 mu m protoplanetary nebula IRAS 06530-0213

arXiv:2607.25304 · astro-ph.GA, astro-ph.SR · Submitted 2026-07-28 · Read on arXiv

Hao-Min Sun, Zhuang Zhang, Jun-Yang Liu, Sheng-Li Qin, Yong Zhang

astro-ph.GA, astro-ph.SR

Submitted: 2026-07-28

Comments: 29 pages, 11 figures, 2 tables. Accepted for AJ

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

Terminology

• Abundance — 24× in this paper · explained in 1 episode
• Trace — 8× in this paper · explained in 2 episodes
• Benchmark — 3× in this paper · explained in 2 episodes
• Calibration — 2× in this paper · explained in 7 episodes
• Asymptotic Giant Branch — 1× in this paper
• Signal-to-noise ratio (SNR) — 1× in this paper · explained in 2 episodes
• Square Kilometre Array — 1× in this paper

Sources

• An accelerated Monte Carlo method to solve two-dimensional radiative transfer and molecular excitation

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