Intergalactic and galactic clouds on the line of sight to SN 1993J in M 81 seen in IUE spectra.
Bomans, D. J.; Fransson, C.; Kirshner, R. P.; Sonneborn, G.; de Boer, K. S.; Wamsteker, W.; Rodriguez Pascual, P.
Germany, Spain, Sweden, United States
Abstract
High resolution IUE spectra of SN 1993J in M81 show the existence of several clouds on the line of sight. These include local galactic gas at 0 km s^-1^, gas in M81 at -130 km s^-1^, a cloud in the halo of the Milky Way near -45 km s^-1^, and an intergalactic cloud near +140 km s^-1^. Arguments for each of these locations are given. There is little gas in M81 in front of SN 1993J and no detectable CIV at or near -130 km s^-1^. The gas of the halo of the Milky Way shows a large amount of CIV and SiIV. The intergalactic cloud shows a large velocity width extending from +100 km s^-1^ to +200 km s^-1^ and is very prominent in the absorption lines of AlIII, SiIV, and CIV. It may be related to energetic events in the M81 group of galaxies.