paper

Relation between activity, morphology and environment for a large sample of SDSS galaxies

arXiv:1011.5286

Abstract

We apply a stellar population synthesis code to the spectra of a large sample of SDSS galaxies to classify these according to their activity (using emission-line diagnostic diagrams), environment (using catalogues of isolated and cluster galaxies), and using parameters that correlate with their morphology.

1 page, 1 figure; to appear in Proceedings of the XIII Latin American Regional IAU Meeting, Morelia, Mexico, 8-12 Nov. 2010

Relation between activity, morphology and environment for a large sample of SDSS galaxies · wovepaper