Dynamo-generated magnetic fields in fast rotating single giants
arXiv:0901.1537 · doi:10.1017/S1743921309031020
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 -- dynamo operating in these giants.
2 pages, 1 figure, proceedings of IAUS259: Cosmic Magnetic Fields
Cited by in corpus (5)
- Discovery of a weak magnetic field in the photosphere of the single giant Pollux
- Direct detection of a magnetic field in the photosphere of the single M giant EK Boo: How common is magnetic activity among M giants?
- Magnetic field structure in single late-type giants: The effectively single giant V390 Aur
- Simultaneous VLBA polarimetric observations of the v=1,2 J=1-0 and v=1, J=2-1 SiO maser emission toward VY CMa II: component-level polarization analysis
- 14 Ceti: A probable Ap-star-descendant entering the Hertzsprung gap