We present deep 450 and 850µ m SCUBA images of the nearby spiral galaxy NGC 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 7331 (TB <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 further 10 galaxies and, collectively, these data indicate TB =0.1 -0.2 at the R(25) radius. Our constraints on disk opacity are fed into a simulation of how light emanating from high redshifts is attenuated by foreground spirals. In making this calculation, we consider the possibility that galactic disks may have also conta...
We present sub-millimetre images of the spiral galaxy NGC 6946 at 450 and 850 mu m. The observations...
The distribution of dust in nearby spiral galaxies not only affects our perceptions of disc morpholo...
The opacity of foreground spiral disks can be probed from the number of distant galaxies seen throug...
We present deep 450 and 850µ m SCUBA images of the nearby spiral galaxy NGC 7331. Using the submilli...
We have analysed SCUBA $850~\mu$m images of the (near) face-on spiral galaxy NGC 6946, paying parti...
We present observations of the spiral galaxy NGC 7331 using the Submillimetre Common User Bolometer ...
12 pages, 9 figuresWe have analysed SCUBA 850\\mum images of the (near) face-on spiral galaxy NGC 69...
This thesis investigates the emission of sub-millimetre-wave radiation from galaxies in the Hubble ...
We compare [FORMULA]m SCUBA images of NGC 891 with the corresponding V-band optical depth predicted ...
Submillimetre mapping observations of the active edge-on spiral galaxy NGC 3079 are presented. These...
We use the radiation transfer simulation of Xilouris et al. ([CITE]) to constrain the quantity of d...
International audienceWe describe a search for submillimeter emission in the vicinity of one of the ...
Dust extinction can be determined from the number of distant field galaxies seen through a spiral di...
We have measured the radial brightness distributions in the disks of three nearby face-on spiral gal...
We have measured the radial brightness distributions in the disks of three nearby face-on spiral gal...
We present sub-millimetre images of the spiral galaxy NGC 6946 at 450 and 850 mu m. The observations...
The distribution of dust in nearby spiral galaxies not only affects our perceptions of disc morpholo...
The opacity of foreground spiral disks can be probed from the number of distant galaxies seen throug...
We present deep 450 and 850µ m SCUBA images of the nearby spiral galaxy NGC 7331. Using the submilli...
We have analysed SCUBA $850~\mu$m images of the (near) face-on spiral galaxy NGC 6946, paying parti...
We present observations of the spiral galaxy NGC 7331 using the Submillimetre Common User Bolometer ...
12 pages, 9 figuresWe have analysed SCUBA 850\\mum images of the (near) face-on spiral galaxy NGC 69...
This thesis investigates the emission of sub-millimetre-wave radiation from galaxies in the Hubble ...
We compare [FORMULA]m SCUBA images of NGC 891 with the corresponding V-band optical depth predicted ...
Submillimetre mapping observations of the active edge-on spiral galaxy NGC 3079 are presented. These...
We use the radiation transfer simulation of Xilouris et al. ([CITE]) to constrain the quantity of d...
International audienceWe describe a search for submillimeter emission in the vicinity of one of the ...
Dust extinction can be determined from the number of distant field galaxies seen through a spiral di...
We have measured the radial brightness distributions in the disks of three nearby face-on spiral gal...
We have measured the radial brightness distributions in the disks of three nearby face-on spiral gal...
We present sub-millimetre images of the spiral galaxy NGC 6946 at 450 and 850 mu m. The observations...
The distribution of dust in nearby spiral galaxies not only affects our perceptions of disc morpholo...
The opacity of foreground spiral disks can be probed from the number of distant galaxies seen throug...