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The origins of the magnetic field in tip-RGB, AGB and post-AGB stars

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arxiv 2407.17421 v1 pith:Z5MGT3P7 submitted 2024-07-24 astro-ph.SR

Renada Konstantinova-Antova , Stefan Georgiev , Agnès Lèbre , Corinne Charbonnel , Ana Palacios , Michel Aurière This is my paper
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keywords magneticstarsfieldfieldsgenerationgiantspost-agbactivity
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During the last decade and a half, the new generation spectropolarimeter Narval at Pic du Midi, France allowed the study of weak magnetic fields in cool giant stars that are fairly evolved after main sequence. We present a short summary on the recent knowledge on the magnetic fields and activity in giants situated in the upper right part of the Hertzsprung-Russel (H-R) diagram and discuss on the possible mechanisms for magnetic field generation in the asymptotic giants branch (AGB) and post-AGB stars.

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Cited by 1 Pith paper

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  1. Atmospheric Signatures of Common Envelope Evolution in White Dwarf Planets

    astro-ph.EP 2026-07 conditional novelty 6.0 of 10

    During common-envelope evolution, engulfed giant planets can accrete enough stellar material to measurably brighten their thermal emission, offering a new atmospheric diagnostic of their dynamical history.

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