[en] We present the results of an abundance analysis of two magnetic B-type stars in the
Orion Nebula Cluster that support the lack of a direct relationship between the existence of a
magnetic field and a nitrogen excess in the photosphere.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Morel, Thierry ; Université de Liège - ULiège > Groupe d'astrophysique des hautes énergies (GAPHE)
Language :
English
Title :
Abundance study of two magnetic B-type stars in the Orion Nebula Cluster
Publication date :
2014
Event name :
IAU Symposium 307 : New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry
