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Density-potential pairs for spherical stellar systems with Sersic light profiles and (optional) power-law cores

Terzic, Balsa; Graham, Alister


Popular models for describing the luminosity-density profiles of dynamically hot stellar systems (e.g. Jaffe, Hernquist, Dehnen) were constructed with the desire to match the deprojected form of an R1/4 light profile. Real galaxies, however, are now known to have a range of different light-profile shapes that scale with mass. Consequently, although highly useful, the above models have implicit limitations, and this is illustrated here through their application to a number of real galaxy density...[Show more]

CollectionsANU Research Publications
Date published: 2005
Type: Journal article
Source: Monthly Notices of the Royal Astronomical Society
DOI: 10.1111/j.1365-2966.2005.09269.x


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