Journal Article

Young ages and other intriguing properties of massive compact galaxies in the local Universe

A. Ferré-Mateu, A. Vazdekis, I. Trujillo, P. Sánchez-Blázquez, E. Ricciardelli and I.G. de la Rosa

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 423, issue 1, pages 632-646
Published in print June 2012 | ISSN: 0035-8711
Published online May 2012 | e-ISSN: 1365-2966 | DOI: http://dx.doi.org/10.1111/j.1365-2966.2012.20897.x
Young ages and other intriguing properties of massive compact galaxies in the local Universe

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We characterize the kinematics, morphology, stellar populations and star formation histories of a sample of massive compact galaxies in the nearby Universe, which might provide a closer look at the nature of their high-redshift (z >rsim 1.0) massive counterparts. We find that nearby compact massive objects show elongated morphologies and are fast rotators. New high-quality long-slit spectra show that they have young mean luminosity-weighted ages (2 Gyr) and metallicities solar or above ([Z/H] >rsim 0.0). No significant stellar population gradients are found. The analysis of their star formation histories suggests that these objects have experienced recently enormous bursts which, in some cases, represent unprecedented large fractions of their total stellar mass. These galaxies seem to be truly unique, as they do not follow the characteristic kinematical and stellar population patterns of present-day massive ellipticals, spirals or even dwarfs.

Keywords: galaxies: abundances; galaxies: evolution; galaxies: formation; galaxies: kinematics and dynamics; galaxies: stellar content

Journal Article.  9191 words.  Illustrated.

Subjects: Astronomy and Astrophysics

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