Witnessing gas mixing in the metal distribution of the Hickson Compact Group HCG 31

Abstract

We present, for the first time, direct evidence that, in a merger of disk galaxies, the preexisting central metallicities will mix as a result of gas being transported in the merger interface region, along the line that joins the two coalescing nuclei. This is shown using detailed 2D kinematics as well as metallicity measurements for the nearby ongoing merger in the center of the compact group HCG 31. We focus on the emission line gas, which is extensive in the system. The two coalescing cores display similar oxygen abundances while in between the two nuclei the metallicity changes smoothly from one nucleus to the other, indicating a mix of metals in this region, which is confirmed by the high resolution H$\alpha$ kinematics (R=45900). This nearby system is especially important because it involves the merging of two fairly low mass and clumpy galaxies (LMC-like galaxies), making it an important system for comparison with high redshift galaxies.

Accepted for publication in the Astrophysical Journal Letters

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Cited by in corpus (5)

• Spatially Resolved Gas-phase Metallicity in FIRE-2 Dwarfs: Late-Time Evolution of Metallicity Relations in Simulations with Feedback and Mergers
• Probing the nature of the pre-merging system Hickson Compact Group 31 through IFU data
• Physical and kinematic conditions of the local merging galaxy NGC 1487
• A MUSE view of the multiple interacting system HCG 31
• MeerKAT view of Hickson Compact Groups:I. Data description and release