SPHERE/ZIMPOL observations of the symbiotic system R Aquarii. II. Dynamics of the dust in the Mira wind and the Halpha gas in the jet
astro-ph.SR, astro-ph.GA
Submitted: 2026-10-04
Updated: 2026-10-04
Sources
- SiO masers and 7 mm Continuum in Mira and R Aqr
- Evolution From Asymptotic Giant Branch to Pre-planetary Nebula: Whorled Patterns and Stellar Companions
- Chemical complexity and dust formation around evolved stars
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