# Resolving the age bimodality of galaxy stellar populations on kpc scales

## TL;DR

This study reveals a bimodal distribution of local stellar ages within galaxies on kpc scales, highlighting distinct old and young regions influenced by galaxy type and internal structures, challenging simple interpretations of galaxy star formation histories.

## Contribution

It provides the first detailed analysis of local age bimodality on kpc scales across a large galaxy sample, linking it to galaxy morphology and internal structures.

## Key findings

- Bimodal local age distribution in galaxy sub-regions.
- Older ages in bulges and inter-arm regions of spirals.
- Identification of an 'old ridge' and a 'young sequence' in age distribution.

## Abstract

Galaxies in the local Universe are known to follow bimodal distributions in the global stellar populations properties. We analyze the distribution of the local average stellar-population ages of 654,053 sub-galactic regions resolved on ~1-kpc scales in a volume-corrected sample of 394 galaxies, drawn from the CALIFA-DR3 integral-field-spectroscopy survey and complemented by SDSS imaging. We find a bimodal local-age distribution, with an old and a young peak primarily due to regions in early-type galaxies and star-forming regions of spirals, respectively. Within spiral galaxies, the older ages of bulges and inter-arm regions relative to spiral arms support an internal age bimodality. Although regions of higher stellar-mass surface-density, mu*, are typically older, mu* alone does not determine the stellar population age and a bimodal distribution is found at any fixed mu*. We identify an "old ridge" of regions of age ~9 Gyr, independent of mu*, and a "young sequence" of regions with age increasing with mu* from 1-1.5 Gyr to 4-5 Gyr. We interpret the former as regions containing only old stars, and the latter as regions where the relative contamination of old stellar populations by young stars decreases as mu* increases. The reason why this bimodal age distribution is not inconsistent with the unimodal shape of the cosmic-averaged star-formation history is that i) the dominating contribution by young stars biases the age low with respect to the average epoch of star formation, and ii) the use of a single average age per region is unable to represent the full time-extent of the star-formation history of "young-sequence" regions.