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Dynamo-generated magnetic fields in fast rotating single giants

2008/11/01 by Renada Konstantinova-Antova, Michel Aurière, Klaus-Peter Schröder +1 · 1 citation
Physics and Astronomy · #Astronomy and Astrophysical Research #Pulsars and Gravitational Waves Research #Stellar, planetary, and galactic studies #astro-ph.SR

paper · pdf · doi:10.1017/s1743921309031020

2 pages, 1 figure, proceedings of IAUS259: Cosmic Magnetic Fields

openalex publication_date 2008/11/01 · arxiv created 2009/01/12 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/04

Abstract

Abstract Red giants offer a good opportunity to study the interplay of magnetic fields and stellar evolution. Using the spectro-polarimeter NARVAL of the Telescope Bernard Lyot (TBL), Pic du Midi, France and the LSD technique we began a survey of magnetic fields in single G-K-M giants. Early results include 6 MF-detections with fast rotating giants, and for the first time a magnetic field was detected directly in an evolved M-giant: EK Boo. Our results could be explained in the terms of α–ω dynamo operating in these giants.

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