The observations analysed here were obtained with the IUE short and long wavelength cameras (SWP and LWP respectively Boggess & Wilson 1987) during 12 consecutive days in September 1992. Several spectra were obtained each day alternating between LWP high resolution and SWP low resolution. A detailed list of observing dates, image numbers and line fluxes at Earth for the most prominent emission lines in each spectrum was included in Paper I as well as a complete description of the observing scheme and the reduction procedure.
© European Southern Observatory (ESO) 2000
Online publication: March 17, 2000