Journal Article

Stellar population gradients in brightest cluster galaxies

S. I. Loubser and P. Sánchez-Blázquez

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 425, issue 2, pages 841-861
Published in print September 2012 | ISSN: 0035-8711
Published online September 2012 | e-ISSN: 1365-2966 | DOI: http://dx.doi.org/10.1111/j.1365-2966.2012.21079.x
Stellar population gradients in brightest cluster galaxies

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Abstract

We present the stellar population and velocity dispersion gradients for a sample of 24 brightest cluster galaxies (BCGs) in the nearby Universe for which we have obtained high-quality long-slit spectra at the Gemini telescopes. With the aim of studying the possible connection between the formation of the BCGs and their host clusters, we explore the relations between the stellar population gradients and properties of the host clusters, as well as the possible connections between the stellar population gradients and other properties of the galaxies. We find mean stellar population gradients (negative Δ[Z/H]/log r gradient of −0.285 ± 0.064, small positive Δlog (age)/log r gradient of 0.069 ± 0.049 and null Δ[E/Fe]/log r gradient of −0.008 ± 0.032) that are consistent with those of normal massive elliptical galaxies. However, we find a trend between metallicity gradients and velocity dispersion (with a negative slope of −1.616 ± 0.539) that is not found for the most massive ellipticals. Furthermore, we find trends between the metallicity gradients and K-band luminosities (with a slope of 0.173 ± 0.081) as well as the distance from the BCG to the X-ray peak of the host cluster (with a slope of −7.546 ± 2.752). The latter indicates a possible relation between the formation of the cluster and that of the central galaxy.

Keywords: galaxies: elliptical and lenticular, cD; galaxies: evolution; galaxies: stellar content

Journal Article.  7986 words.  Illustrated.

Subjects: Astronomy and Astrophysics

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