Deep submillimeter images of NGC 7331; dust at the periphery of spiral disks

We present deep 450 and 850 mum SCUBA images of the nearly spiral galaxy NG C 7331. Using the submillimeter emissivity inferred from COBE observations of Milky Way dust, we convert our SCUBA images into maps of optical depth. The opacity derived in this way is quite low at the visible limit of NGC 73 31 (tau (B) less than or equal to 0.22 at the R-25 radius for the disk seen face-on). In a similar fashion, we exploit SCUBA and ISOPHOT images of a f urther 10 galaxies and, collectively, these data indicate tau (B) = 0.1-0.2 at the R-25 radius. Our constraints on disk opacity are fed into a simulat ion of how light emanating from high redshifts is attenuated by foreground spirals. In making this calculation, we consider the possibility that galac tic disks may have also contained different dust masses in the past. We est imate that less than 10% of the light emitted by Hubble Deep Field galaxies fails to reach the B-band observer due to intervening spirals.