Abstract
Etude des proprietes des boucles coronales de longueur comparable au rayon des etoiles de la sequence principale en rotation rapide telle que AB Doradus. Des modeles numeriques sont developpes pour traiter les equations d'equilibre des boucles statiques. Les temperatures de plasma et les densites d'electron obtenues sont en accord avec les observations RX de l'etoile. Les variations de densite dans la boucle sont evaluees et l'influence de la gravitation est analysee
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