Absorption line systems on the line of sight from SN 1987A to SN 1993J andthe intergalactic cloud in front of M 81

We present an extended analysis of the high dispersion IUE spectra of SN 19 93J in M81, based on the improved data in the IUE final archive. Eight inte rstellar absorption components can be identified in the velocity range from -200km s(-1) to +200 km s(-1). Column densities are determined for Fe II, ME I, Mg Ir, O I, S II, Si Ir, and Zn II. From the ion ratios, we estimate electron densities and temperatures of the gas in these components. In addi tion, we rederive column density profiles for the higher ionisation stages Al III, Si Iv, and Cry for the entire line of sight. Of special interest are the absorption components at positive velocities, w hich are associated with the intergalactic medium (IGM) in the foreground o f M81. The medium has many gas components, as known from radio measurements , probably released in dynamical interactions by galaxies in the M81 group. The IUE spectra contain the only UV absorption information on such gas. We find neutral and ionised gas absorption at the same velocity, having a met al content similar to a galactic disk. We combine the spectra towards SN1993J in M81 with those towards SN 1987A i n the LMC, the directions being essentially antipodes on the celestical sph ere. Comparing the total profile with QSO spectra, we conclude that most ab sorption in QSO spectra occurs in diffuse clouds on those sight lines and i s not similar to absorption by galactic disk gas. However, one absorption c omponent towards SN 1993J is clearly very similar to some of the absorption components in QSO spectra.