Periodic activity on the (sub)mm surface of the AGB star Mira A

arXiv:2608.23724 · astro-ph.SR · Submitted 2026-08-24 · Read on arXiv

astro-ph.SR

Submitted: 2026-08-24

Updated: 2026-08-24

Comments: Submitted to A&A, with most comments from the 1st round of review implemented

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

Terminology

• Asymptotic Giant Branch — 3× in this paper
• Degeneracy — 3× in this paper · explained in 3 episodes
• Trace — 2× in this paper · explained in 2 episodes
• Aperture — 1× in this paper · explained in 1 episode
• Calibration — 1× in this paper · explained in 7 episodes
• Common Astronomy Software Applications — 1× in this paper
• Cooperation — 1× in this paper · explained in 2 episodes
• European Southern Observatory — 1× in this paper
• Frequency Dependence — 1× in this paper · explained in 2 episodes

Sources

• VLTI-GRAVITY measurements of cool evolved stars: II. Pulsation properties and mass-loss process of the Mira star R Car and the red supergiant VX Sgr

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