Deprojection of the de Vaucouleurs R exp 1/4 brightness profile

Details Deprojection of the de Vaucouleurs R exp 1/4 brightness profile Deprojection of the de Vaucouleurs R exp 1/4 brightness profile

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...175....1m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 175, no. 1-2, March 1987, p. 1-3.

Statistics

Computation

48

Brightness, Galactic Clusters, Gravitational Fields, Luminosity, Computational Astrophysics, Galactic Structure, Halos, Numerical Analysis, Spatial Distribution

Scientific paper

A tractable analytical expression is given which very closely approximates a deprojected r exp 1/4 brightness profile. It can be useful for a variety of applications, such as numerical simulations of gravitational systems with an r exp 1/4 brightness profile. The method is illustrated by deducing an analytical three-dimensional luminosity profile of the Coma cluster of galaxies.

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