[en] Despite their relatively large incidence among early-type stars, only a few B-stars have been
observed with X-ray gratings. We therefore undertook a legacy project with XMM to gather high-
resolution spectra of a set of early B stars selected on the basis of their high RASS count rate.
This poster presents the preliminary results of this project.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Nazé, Yaël ; Université de Liège - ULiège > Groupe d'astrophysique des hautes énergies (GAPHE)
Cazorla, C.
Rauw, Grégor ; Université de Liège - ULiège > Groupe d'astrophysique des hautes énergies (GAPHE)
Morel, Thierry ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie
