In the adult Sprague–Dawley rat retina, very few cells were
dying; only the occasional cell was TUNEL
+ (red
in
Fig. 2A ). Higher densities of TUNEL
+ profiles (as in
Fig. 2B ) resulted from damaging stimuli, in this case 24 hours of BCL.
Astrocytes (identified by their GFAP content, red in
Fig. 2C ) were
largely confined to the inner surface. bFGF (green in
Figs. 2C 2D 2E 2F 2G 2H 2I ) was prominent in somas in the inner nuclear layer (INL; i in
Fig. 2C ) and in astrocyte nuclei (e.g., top of
Fig. 2C ). At the peripheral
edge of the retina (
Fig. 2D , lower arrow) bFGF was prominent in the
outer nuclear layer (ONL; o in
Fig. 2 ) and, toward the edge (between
the arrows in
Fig. 2D ), GFAP expression (red) in Müller cells
appeared upregulated. The presence of GFAP in Müller cell
processes is an index of environmental,
19 20 21 genetic,
19 22 and mechanical
11 23 24 25 stress.
The co-upregulation of bFGF in the ONL and of GFAP in Müller
cells was normally apparent only at the edge of the retina but could be
elicited in midperipheral retina by exposure to BCL
(Fig. 2E) . In
favorable preparations of unstressed retina, bFGF protein could be seen
in the end feet of Müller cells (
Fig. 2F , vertical arrow) as well
as astrocyte nuclei (oblique arrow). The Müller cell processes,
labeled for vimentin (red) in
Figures 2F 2G and 2H , could be followed
to bFGF-laden somas in the INL. At higher power
(Fig. 2H) each vimentin
bundle could be seen to skirt or split around a bFGF-laden profile,
suggesting that the bFGF profile was the nucleus of a Müller
cell. Around retinal vessels
(Fig. 2I) , the astrocytic glia limitans
was GFAP
+ (red). bFGF was prominent in astrocyte
nuclei (
Fig. 2I , arrows), and a blush of green labeling inside the glia
limitans indicated the presence of bFGF protein in the endothelial
cells of the vessel wall.