We outline the results of a two-dimensional (2D) fit to the light distribution of early-type galaxies belonging to a complete volume-limited sample and discuss briefly the significant correlations among the structural parameters. In particular we reconfirm that the lack of structural homology is probably a characteristic of hot stellar systems.

Structure of Early-Type Galaxies

D'ONOFRIO, MAURO;
2001

Abstract

We outline the results of a two-dimensional (2D) fit to the light distribution of early-type galaxies belonging to a complete volume-limited sample and discuss briefly the significant correlations among the structural parameters. In particular we reconfirm that the lack of structural homology is probably a characteristic of hot stellar systems.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11577/1343599
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