Published in "QSO Absorption Lines", Space Telescope Science Institute Symposium Series 2, 1987, eds. J. C. Blades, D. A. Turnshek and C. A. Norman


DAMPED Ly-ALPHA ABSORPTION SYSTEMS

Arthur M. Wolfe

Mt. Wilson and Las Campanas Observatory and the University of Pittsburgh


Abstract. QSO absorption systems with damped Ly-α lines belong to a distinct population of absorbers with properties that bring to mind the HI disks of spiral galaxies. A survey for damped Ly-α systems is described. It is shown that they occur more frequently along the line-of-sight than do normal spiral galaxies. The damped systems contribute a mass density per unit comoving volume that (a) dominates the baryon content of the universe at redshifts z = 2 - 3, and (b) is comparable to the mass per unit comoving volume contributed by luminous matter in present-day spiral galaxies. It is suggested that the damped absorbers are large HI disks which are the progenitors of normal spiral galaxies.


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