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

TL;DR

This study uses PCA on SDSS early-type galaxy spectra to identify new indicators of age and recent star formation, revealing environmental influences on galaxy evolution.

Contribution

It introduces new PCA-based parameters, eta and zeta, to quantify stellar age and recent star formation, providing insights into environmental effects.

Findings

Zeta is sensitive to recent star formation episodes.

Eta correlates with average stellar age.

Galaxies in low-density regions show less recent star formation.

Abstract

(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.).