Decoding the spectra of SDSS early-type galaxies: New indicators of age and recent star formation

Details Decoding the spectra of SDSS early-type galaxies: New indicators of age and recent star formation Decoding the spectra of SDSS early-type galaxies: New indicators of age and recent star formation

2007-09-03

arxiv.org/abs/0709.0300v1

Mon.Not.Roy.Astron.Soc. 382 (2007) 750-760

Astronomy and Astrophysics

Astrophysics

19 pages, 12 figures. Accepted for publication in MNRAS

Scientific paper

10.1111/j.1365-2966.2007.12446.x

(Abridged) We apply Principal Component Analysis (PCA) to a sample of early-type galaxies from the Sloan Digital Sky Survey (SDSS) in order to infer differences in their star formation histories. Out of the first few principal components (PC), we study four which give information about stellar populations and velocity dispersion. We construct two parameters (eta and zeta) as linear combinations of PC1 and PC2. We find zeta to be most sensitive to recent episodes of star formation, and eta to be strongly dependent on the average age of the stellar populations. The distribution of the eta component of the composites appear to be indistinguishable between high and low density regions, whereas the distribution of zeta parameters have a significant skew towards lower values for galaxies in low density regions. This result suggests that galaxies in lower density environments are less likely to present weak episodes of recent star formation. In contrast, a significant number of galaxies from our high density subsample -- which includes clusters (both outer regions and centres) and groups -- underwent small but detectable recent star formation at high metallicity, in agreement with recent estimates targeting elliptical galaxies in Hickson Compact Groups and in the field (Ferreras et al.).

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