# Interaction effects on galaxy pairs with GeminiGMOS-III: Stellar population synthesis

## TL;DR

This study investigates how galaxy interactions influence stellar populations, revealing that interacting galaxies often have younger stars and higher star formation activity compared to isolated galaxies, with secondary galaxies showing more young stars.

## Contribution

It provides new insights into the impact of galaxy interactions on stellar populations using Gemini GMOS spectra and stellar population synthesis, highlighting differences from isolated galaxies.

## Key findings

- Interacting galaxies are dominated by young/intermediate stellar populations.
- Secondary galaxies tend to have higher contributions of young stars.
- Nebular extinctions are about twice the stellar extinctions.

## Abstract

We present an observational study of the impacts of the interactions on the stellar population in a sample of galaxy pairs. Long-slit spectra in the wavelength range 3440-7300 {\AA} obtained with the Gemini Multi-Object Spectrograph (GMOS) at Gemini South for fifteen galaxies in nine close pairs were used. The spatial distributions of the stellar population contributions were obtained using the stellar population synthesis code STARLIGHT. Taking into account the different contributions to the emitted light, we found that most of the galaxies in our sample are dominated by the young/intermediate stellar populations. This result differs from the one derived for isolated galaxies where the old stellar population dominates the disc surface brightness. We interpreted such different behavior as being due to the effect of gas inflows along the disk of interacting galaxies on the star formation in a time scale of the order of about 2Gyr. We also found that, in general, the secondary galaxy of the pairs has a higher contribution of the young stellar population than the primary one. We compared the estimated values of the stellar and nebular extinctions derived from the synthesis method and the H{\alpha}/H\b{eta} emission-line ratio finding that the nebular extinctions are systematically higher than stellar ones by about a factor of 2. We did not find any correlation between nebular and stellar metallicities. We neither found a correlation between stellar metallicities and ages while a positive correlation between nebular metallicities and stellar ages was obtained, with the older regions being the most metal-rich.