The Ultraviolet Spectrum of the Be-Star 88-HERCULIS

Abstract

In this paper, we give a detailed list and analysis of line identifications of the UV spectrum of the Be star 88 Her in the wavelength range λλ1958–3002 Å recorded in 1984, 23 May with the International Ultraviolet Explorer (IUE). The spectrum is crowded by shell absorptions lines, mostly those of singly ionized iron peak elements. The detailed analysis of the radial velocities measured in the whole spectral range 1100–3002 Å is also given.