The First Integral Field Unit Spectroscopic View of Shocked Cluster Galaxies

Abstract

Galaxy clusters grow by merging with other clusters, giving rise to Mpc-wide shock waves that travel at 1000-2500 km/s through the intra-cluster medium. To study the effects of merger shocks on the properties of cluster galaxies, we present the first spatially resolved spectroscopic view of 5 H$\alpha$ emitting galaxies located in the wake of shock fronts in the low redshift (z~0.2), massive (~2$\times 10^{15}$ M${}_{\odot }$), post-core passage merging cluster, CIZA J2242.8+5301 (nicknamed the `Sausage'). Our Gemini/GMOS-N integral field unit (IFU) observations, designed to capture H$\alpha$ and [NII] emission, reveal the nebular gas distribution, kinematics and metallicities in the galaxies over >16 kpc scales. While the galaxies show evidence for rotational support, the flux and velocity maps have complex features like tails and gas outflows aligned with the merger axis of the cluster. With gradients incompatible with inside-out disk growth, the metallicity maps are consistent with sustained star formation (SF) throughout and outside of the galactic disks. In combination with previous results, these pilot observations provide further evidence of a likely connection between cluster mergers and SF triggering in cluster galaxies, a potentially fundamental discovery revealing the interaction of galaxies with their environment.

Published in ApJ Letters. Main results can be found in Figure 3. Data behind figures are available together with the journal paper

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• The XXL Survey XLV. Linking the ages of optically selected groups to their X-ray emission
• XXL-HSC: Host properties of X-ray detected AGNs in XXL clusters
• GLEAM: Galaxy Line Emission & Absorption Modeling