The Luminous Matter Profiles in Ellipticals since boldmath{z˜1.5}: The Photometric Plane and its Evolution

Details The Luminous Matter Profiles in Ellipticals since boldmath{z˜1.5}: The Photometric Plane and its Evolution The Luminous Matter Profiles in Ellipticals since boldmath{z˜1.5}: The Photometric Plane and its Evolution

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..390..498o&link_type=abstract

Pathways Through an Eclectic Universe ASP Conference Series, Vol. 390, proceedings of the conference held 23-27 April, 2007 at S

Mathematics

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Scientific paper

We present results of an analysis of the stellar mass distributions of
relaxed elliptical-like objects (ELOs) identified, at z=0, z=0.5, z=1,
and z=1.5, in a set of self-consistent hydrodynamical simulations
operating in the context of a concordance cosmological model, confirming
the existence of a photometric plane, as observations suggest.

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