Relation between activity, morphology and environment for a large sample of SDSS galaxies
Cosmology and Nongalactic Astrophysics
2010-11-25 v1
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.
Keywords
Cite
@article{arxiv.1011.5286,
title = {Relation between activity, morphology and environment for a large sample of SDSS galaxies},
author = {R. A. Ortega-Minakata and J. P. Torres-Papaqui and H. Andernach and J. M. Islas-Islas and D. M. Neri-Larios},
journal= {arXiv preprint arXiv:1011.5286},
year = {2010}
}
Comments
1 page, 1 figure; to appear in Proceedings of the XIII Latin American Regional IAU Meeting, Morelia, Mexico, 8-12 Nov. 2010