The heavy-element redshifts are thought to be due to intervening galaxies. The lines of evidence in favor of this hypothesis are as follows.
0.8. Several
impressive cases of such
galaxies are detailed in the survey article by
Bergeron (1988).
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: