2023RNAAS...7..111M

The analysis of the far-ultraviolet spectrum of the B9 Si HD 215441 recorded by the LWRS camera on board FUSE reveals a large deficiency of the flux when compared to the non-magnetic late B-type star HD 182308 of similar fundamental parameters. Most features can be identified using spectrum synthesis. The FUSE spectrum of HD 215441 contains mostly blends of low-excitation lines of Ti II, Mn II, Cr II, Fe II, a few lines of Ti III, Cr III and Fe III and interesting lines of C III, P II, S II and Cl I.