The heavy-element redshifts are thought to be due to intervening galaxies. The lines of evidence in favor of this hypothesis are as follows.
The frequency of absorption systems of a given type may be used to infer the
required mean cross-section for absorbers of different types, assuming
that the
Schechter (1976)
function describes the distribution over galaxy luminosities and
that the radius
of a galaxy is related to its luminosity in the same manner as the
Holmberg radius,
namely R
L5/12. With these assumptions the effective
radius, R*, of an L* galaxy
comes out to be 75 kpc for the Lyman limit systems, 50 kpc for the MgII
systems, 90 kpc for the CIV systems and 480 kpc for the
Ly-
clouds, supposing
that they
originate in galaxies. These numbers, which were given to me by Tytler (1986,
private communication), are evaluated for a mean redshift of z =
2.5, for H0 = 100 km
s-1 Mpc-1 and include only spiral galaxies. As is
well known, these effective
cross-sections are much larger than the optical sizes of galaxies at the
present epoch. Also, according to
Tytler (1987a)
there are 6 times as many Lyman limit absorbers with
N(HI)
3.0 x 1018
cm-2 at z = 2 than are
seen locally in 21 cm measurements. In a similar vein,
Wolfe (1988)
has deduced that there are five times as many
damped Ly-
absorbers (presumed to be galactic disks) with N(HI) > 2.0 x
1020 cm-2 at z = 2.6
than there are locally per unit co-moving volume. These observations may
constitute
evidence for substantial evolution of galactic disks in relatively
recent epochs.
A critical question concerning the heavy-element redshifts is the origin of the velocity structure. Three types of possible origin have been proposed: