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Paper: Do All Galaxies Have Disks (and are Some Small)?
Volume: 230, Galaxy Disks and Disk Galaxies
Page: 153
Authors: Burstein, D.; Saglia, R. P.; Colless, M.; Davies, R. L.; McMahan, R. K.; Wegner, G.
Abstract: We fit luminosity profiles to a large sample of cluster galaxies chosen to be strongly biased against spiral galaxies. We detect exponential components in 87% of these galaxies, and infer that the remaining cases are consistent with low surface brightness disks contributing less than 10% of the total luminosity. We note various lines of evidence indicating that these exponential components are most rotationally-supported disks, with perhaps more thickened disks in cD galaxies. We suggest that all galaxies possess a disk component, although 20% are not actively forming stars, and a small fraction are too faint to see against a much more luminous bulge component.
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