Considérations sur les raies interdites de [Fe II], [Fe III], [Ni II] et [Ni III] observables dans les étoiles Be, par véhicules spatiaux

Abstract

The strongest forbidden transitions of [Fe II], [Fe III], [Ni II] and [Ni III] have been computed as a preliminary step in the preparation of spectroscopic observations of bright line stars with space vehicles. Several predicted forbidden emissions play certainly an important role, especially in the infrared region.