Damped Ly alpha absorption from a nearby low surface brightness galaxy

Ground-based and Hubble Space Telescope (HST) images of the nearby galaxy S BS 1543+593 (z = 0.009) show it to be a low surface brightness (LSB) galaxy with a central surface brightness mu (B)(0) = 23.2 mag arcsec(-2) and scal e length 0.9 h(100)(-1) kpc, values typical for the local LSB galaxy popula tion. The galaxy lies directly in front of the quasi-stellar object HS 1543 +5921 (z = 0.807); an HST STIS spectrum of the quasar reveals a damped Ly a lpha (DLy alpha) line at the redshift of the interloper with an H I column density of log N(H I) = 20.35, as well as several low-ionization metal line s with strengths similar to those found in the Milky Way interstellar mediu m. Our data show that LSB galaxies are certainly able to produce the DLy al pha lines seen at higher redshift and fuels the speculation that LSB galaxi es are a major contributor to that population of absorbers.