A giant magnetic eruption from the asymptotic-giant-branch star Mira A

Mass loss during the advanced evolutionary stages of low- and intermediate-mass stars is traditionally attributed to dust-driven winds, whereas the influence of magnetic fields remains poorly constrained. However, recent observations show massive directional mass ejections from the nearby asymptotic-giant-branch (AGB) star Mira A that do not appear to be driven by radiation pressure on the dust. We aim to observationally investigate whether magnetic fields are responsible for the mass-loss ejections from Mira A. We obtained full-polarisation ALMA observations of the SiO v=1, J=5̊ightarrow4 maser transition at 215 GHz with angular resolutions of 1.5--2.6 au. The observations reveal a highly magnetised loop-like mass ejection traced by strongly polarised SiO masers extending to approximately eight stellar radii. The morphology, polarisation pattern, energetics, and kinematics indicate a magnetically driven eruption analogous to a stellar coronal-mass ejection (CME). These observations demonstrate that magnetic eruptions can dominate mass loss from evolved stars and imply that magnetic fields must become an integral component of future models of AGB (and potentially other cool-giant) winds.

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Publication Details

Journal
Astronomy and Astrophysics
Published
2026-10-29
DOI
https://doi.org/10.1051/0004-6361/202662604
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
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article

A giant magnetic eruption from the asymptotic-giant-branch star Mira A

T. Khouri, Sven Wedemeyer, Behzad Bojnordi Arbab, L. Planquart et al.
1 links
Astronomy and Astrophysics
Stellar, planetary, and galactic studies
article

A giant magnetic eruption from the asymptotic-giant-branch star Mira A

T. Khouri, Sven Wedemeyer, Behzad Bojnordi Arbab, L. Planquart, E. De Beck, M. Maercker, M. Andriantsaralaza, Markus Wittkowski, Hans Olofsson, W. H. T. Vlemmings, R. Unnikrishnan, M. Saberi, S del Palacio, D. Jadlovský, B. Lankhaar, M. Siebert, E. Humphreys
article en

Abstract

Mass loss during the advanced evolutionary stages of low- and intermediate-mass stars is traditionally attributed to dust-driven winds, whereas the influence of magnetic fields remains poorly constrained. However, recent observations show massive directional mass ejections from the nearby asymptotic-giant-branch (AGB) star Mira A that do not appear to be driven by radiation pressure on the dust. We aim to observationally investigate whether magnetic fields are responsible for the mass-loss ejections from Mira A. We obtained full-polarisation ALMA observations of the SiO v=1, J=5̊ightarrow4 maser transition at 215 GHz with angular resolutions of 1.5--2.6 au. The observations reveal a highly magnetised loop-like mass ejection traced by strongly polarised SiO masers extending to approximately eight stellar radii. The morphology, polarisation pattern, energetics, and kinematics indicate a magnetically driven eruption analogous to a stellar coronal-mass ejection (CME). These observations demonstrate that magnetic eruptions can dominate mass loss from evolved stars and imply that magnetic fields must become an integral component of future models of AGB (and potentially other cool-giant) winds.

Astronomy and Astrophysics
National Science Foundation, National Radio Astronomy Observatory, European Commission, Korea Astronomy and Space Science Institute, Stiftelsen Olle Engkvist Byggmästare, Norges Forskningsråd, National Astronomical Observatory of Japan, National Science and Technology Council, HORIZON EUROPE Framework Programme, National Institutes of Natural Sciences
Openalex Percentile: Top 34%
Stellar, planetary, and galactic studies
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