Intrinsic versus observed properties in near large spherical structures

Details Intrinsic versus observed properties in near large spherical structures Intrinsic versus observed properties in near large spherical structures

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...209...15j&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 209, no. 1-2, Jan. 1989, p. 15-20. Research supported by the Direccion General

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Computational Astrophysics, Galactic Clusters, Galactic Structure, Local Group (Astronomy), Elliptical Galaxies, Galactic Evolution, Stellar Evolution

Scientific paper

The effects of projection on the observed characteristics of spherically symmetric galactic structures have been studied with respect to the luminosity behavior and the radial dependence of scalar properties. It is demonstrated that inversion of projected two-dimensional radial profiles is not possible except in the case of negligible luminosity segregation. The present inverse method is shown to be well suited for the study of near spherical galaxy systems (such as the Local Supercluster) which are endowed with a Schechter (or Abell) type luminosity function.

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