Magnetism in Cool Evolved Stars

This Thesis presents a study of five magnetically active cool evolved stars of different spectral types and different evolutionary status. All the stars are studied using long-term monitoring in high resolution spectropolarimetry obtained with the instrument Narval and its successor, NeoNarval, inst...

Full description

Bibliographic Details
Main Author: Mikhov, Stefan Georgiev
Other Authors: Laboratoire Univers et Particules de Montpellier (LUPM), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Université Montpellier, Institute of Astronomy and National Astronomical Observatory, Bulgarian Academy of Sciences, Sofia, Agnès Lebre, Renada Konstantinova-Antova
Format: Doctoral or Postdoctoral Thesis
Language:French
Published: HAL CCSD 2021
Subjects:
Stellar Magnetism
Cool Evolved Stars
Stellar Evolution
Magnétisme Stellaire
Étoiles Froides Évoluées
Évolution Stellaire
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Ari
narval
Online Access:https://theses.hal.science/tel-03599880
https://theses.hal.science/tel-03599880/document
https://theses.hal.science/tel-03599880/file/GEORGIEV_2021_archivage.pdf

Similar Items