Interstellar lines in the ultraviolet spectrum of delta Scorpii

Results of a study of the interstellar resonance lines of the cosmologically most abundant elements with the aid of a spectrograph sensitive in the range from 1150 to 1700 A. These lines were analyzed by curve-of-growth techniques to yield column densities from which abundances relative to atomic hydrogen were determined. With the exception of silicon, the relative abundances of the detected species for which column densities could be determined are less by a factor of 1.8 to 8.6 than the relative solar abundances. Silicon, on the other hand, is slightly overabundant by a factor of 1.6.