Star Formation Properties in Barred Galaxies(SFB). I. Ultraviolet-to-Infrared Imaging and Spectroscopic Studies of NGC 7479

TL;DR

This study investigates star formation in the barred galaxy NGC 7479 using multi-wavelength data, revealing how a stellar bar and minor merger influence star formation patterns and galaxy evolution.

Contribution

It provides a detailed multi-wavelength analysis of star formation in NGC 7479, highlighting the effects of a stellar bar and minor merger on galaxy evolution.

Findings

Star formation mainly occurs along the bar and arms.

Strong star formation in the bar occurred about 100 Myr ago.

NGC 7479 may be in a transitional evolutionary stage.

Abstract

Large-scale bars and minor mergers are important drivers for the secular evolution of galaxies. Based on ground-based optical images and spectra as well as ultraviolet data from the Galaxy Evolution Explorer and infrared data from the Spitzer Space Telescope, we present a multi-wavelength study of star formation properties in the barred galaxy NGC 7479, which also has obvious features of a minor merger. Using various tracers of star formation, we find that under the effects of both a stellar bar and a minor merger, star formation activity mainly takes place along the galactic bar and arms, while the star formation rate changes from the bar to the disk. With the help of spectral synthesis, we find that strong star formation took place in the bar region about 100 Myr ago, and the stellar bar might have been $\sim$10 Gyr old. By comparing our results with the secular evolutionary scenario from Jogee et al., we suggest that NGC 7479 is possibly in a transitional stage of secular evolution at present, and it may eventually become an earlier type galaxy or a luminous infrared galaxy. We also note that the probable minor merger event happened recently in NGC 7479, and we find two candidates for minor merger remnants.