The relation between dynamics and star formation in barred galaxies
Eric E. Mart\'inez-Garc\'ia, Rosa A. Gonz\'alez-L\'opezlira

TL;DR
This study investigates the connection between star formation and galaxy dynamics in barred spiral galaxies by analyzing color and age gradients, deriving pattern speeds, and comparing them with theoretical expectations.
Contribution
It introduces a method to link observed star formation gradients with galaxy dynamics, estimating pattern speeds and resonance locations in barred galaxies.
Findings
Color/age gradients suggest star formation triggering in bars and spirals.
Derived pattern speeds tend to overestimate true speeds near corotation due to non-circular motions.
Most galaxies show similar pattern speeds for bars and spirals, indicating linked dynamics.
Abstract
We analyze optical and near-infrared data of a sample of 11 barred spiral galaxies, in order to establish a connection between star formation and bar/spiral dynamics. We find that 22 regions located in the bars, and 20 regions in the spiral arms beyond the end of the bar present azimuthal color/age gradients that may be attributed to star formation triggering. Assuming a circular motion dynamic model, we compare the observed age gradient candidates with stellar populations synthesis models. A link can then be established with the disk dynamics that allows us to obtain parameters like the pattern speed of the bar or spiral, as well as the positions of resonance radii. We subsequently compare the derived pattern speeds with those expected from theoretical and observational results in the literature (e.g., bars ending near corotation). We find a tendency to overestimate bar pattern speeds…
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