Evolution of the magnetic field of Betelgeuse from 2009 - 2017
P. Mathias, M. Auri\`ere, A. L\'opez Ariste, P. Petit, B. Tessore, E., Josselin, A. L\`ebre, J. Morin, G. Wade, F. Herpin, A. Chiavassa, M., Montarg\`es, R. Konstantinova-Antova, P. Kervella, G. Perrin, J.-F. Donati,, J. Grunhut

TL;DR
This study monitors Betelgeuse's weak surface magnetic field over 7.5 years, revealing its evolution and linking it to giant convection cells and long secondary periods, using high-quality spectropolarimetric data.
Contribution
It provides the first long-term spectropolarimetric analysis of Betelgeuse's magnetic field, connecting polarization variations to giant convection cells and stellar activity.
Findings
Confirmed the magnetic nature of Betelgeuse's surface with ~1G field.
Identified long secondary period (~2000 days) as dominant in polarization variations.
Linked polarization signatures to giant convection cells as the main origin.
Abstract
Betelgeuse is an M-type supergiant that presents a circularly polarized (Stokes V) signal in its line profiles, interpreted in terms of a surface magnetic field. The weak circular polarization signal has been monitored over 7.5 years in order to follow its evolution on different timescales, and eventually to determine its physical origin. Linear polarization measurements have also been obtained regularly in the last few years. We used both the ESPaDOnS and Narval spectropolarimeters to obtain high signal-to-noise ratio (S/N) spectra, which were processed by means of the least-squares deconvolution (LSD) method. In order to ensure the reality of the very weak circular polarization, special care has been taken to limit instrumental effects. In addition, several tests were performed on the Stokes V signal to establish its stellar and Zeeman origin. We confirm the magnetic nature of…
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