Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.239..939d&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 239, Aug. 15, 1989, p. 939-976.
Astronomy and Astrophysics
Astronomy
252
Optical Thickness, Spiral Galaxies, Astronomical Models, Brightness Distribution, Gas Density, Infrared Astronomy Satellite, Mass To Light Ratios, Surface Properties
Scientific paper
The classical optical evidence for the low optical depths traditionally assigned to spiral disks is reexamined, suggesting that it is highly model-dependent and unconvincing. In particular, layered models with a physically thin but optically thick dust layer behave like optically thin disks. The opposite hypothesis, that such disks are optically thick is then examined in the light of modern evidence. It is found to be consistent with the near IR and IRAS observations, with the surface brightnesses, with the H I and CO column densities and with the H-alpha measurements.
Davies Jonathan
Disney Michael
Phillipps Steven
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