0000000000302968

AUTHOR

Anna Ferré-mateu

showing 2 related works from this author

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

2012

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 c…

PhysicsStellar massStellar populationStar formationmedia_common.quotation_subjectAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGalaxySpectral lineUniverseSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Galaxy Astrophysicsmedia_commonMonthly Notices of the Royal Astronomical Society
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The intriguing properties of local compact massive galaxies: What are they?

2012

AbstractStudying the properties of the few compact massive galaxies that exist in the local Universe (Trujillo et al. 2009) might provide a closer look to the nature of their high redshift (z ≥ 1.0) massive counterparts. By this means we have characterized their main kinematics, structural properties, stellar populations and star formation histories with a set of new high quality spectroscopic and imaging data (Ferré-Mateu et al. 2012 and Trujillo et al. 2012). These galaxies seem to be truly unique, as they do not follow the characteristic kinematics, stellar surface mass density profiles and stellar population patterns of present-day massive ellipticals or spirals of similar mass. They ar…

Luminous infrared galaxyPhysicsSpace and Planetary ScienceGalaxy groupElliptical galaxyAstronomy and AstrophysicsAstrophysicsDiscBrightest cluster galaxyLenticular galaxyGalaxy clusterPeculiar galaxy
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