The SAURON project - VI. Line strength maps of 48 elliptical and lenticular galaxies

Details The SAURON project - VI. Line strength maps of 48 elliptical and lenticular galaxies The SAURON project - VI. Line strength maps of 48 elliptical and lenticular galaxies

2006-02-08

arxiv.org/abs/astro-ph/0602192v1

Mon.Not.Roy.Astron.Soc.369:497-528,2006

Astronomy and Astrophysics

Astrophysics

33 pages, 28 figures. Accepted for publication in MNRAS. A version with full resolution figures is available at http://www.s

Scientific paper

10.1111/j.1365-2966.2006.10153.x

We present absorption line strength maps of 48 representative elliptical and lenticular galaxies obtained as part of the SAURON survey of nearby galaxies. Using high-quality spectra, spatially binned to a constant signal-to-noise, we measure four key age, metallicity and abundance ratio sensitive indices from the Lick/IDS system over a two-dimensional field extending up to approximately one effective radius. We modify the classical Fe5270 index to define a new index, Fe5270S, which maximizes the usable spatial coverage of SAURON. Maps of Hbeta, Fe5015, Mgb and Fe5270S are presented for each galaxy. We use the maps to compute average line strengths integrated over circular apertures of one-eighth effective radius, and compare the resulting relations of index versus velocity dispersion with previous long-slit work. The metal line strength maps show generally negative gradients with increasing radius roughly consistent with the morphology of the light profiles. Remarkable deviations from this general trend exist, particularly the Mgb isoindex contours appear to be flatter than the isophotes of the surface brightness for about 40% of our galaxies without significant dust features. Generally these galaxies exhibit significant rotation. We infer from this that the fast-rotating component features a higher metallicity and/or an increased Mg/Fe ratio as compared to the galaxy as a whole. The Hbeta maps are typically flat or show a mild positive outwards radial gradient, while a few galaxies show strong central peaks and/or elevated overall Hbeta-strength likely connected to recent star-formation activity. For the most prominent post-starburst galaxies even the metal line strength maps show a reversed gradient. (abridged)

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