The Relation Between Stellar Populations and Light Profiles in Early-Type Galaxies

Bibcode
2005mmgf.conf..469V
DOI
10.1007/10995020_113
Vazdekis, Alexandre; Trujillo, Ignacio; Yamada, Yoshihiko
Referencia bibliográfica

Multiwavelength mapping of galaxy formation and evolution, Proceedings of the ESO Workshop held at Venice, Italy, 13-16 October 2003. Edited by A. Renzini and R. Bender. Series Editor: Bruno Leibundgut, ESO, Garching, Germany. ESO astrophysics symposia. Library of Congress Catalog Card No. 2005925391. ISBN 10 3-540-25665-2; ISBN 13 978-540-25565-6; QB857.5.E96 E78 2003. Published by Springer, Berlin, 2005, p.469

Fecha de publicación:
0
2005
Número de autores
3
Número de autores del IAC
1
Número de citas
0
Número de citas referidas
0
Descripción
Early-type (E/SO) galaxies follow tight relations such as the Fundamental Plane, the Color-Magnitude Relation or the Mg2-σ relation (Bender et al. 1992). However little is known about the relation between their morphological shapes and stellar populations (Conselice 2003), most likely because these two fields rely on methods that have grown up separately. Here we explore possible correlations between the Sérsic index n, and relevant stellar population parameters.
Tipo
Sin árbitro

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