The role of cluster mergers and travelling shocks in shaping the H$\alpha$ luminosity function at $\mathbf{z}\sim 0.2$: `sausage' and `toothbrush' clusters

Abstract

The most extreme cluster mergers can lead to massive cluster-wide travelling shock waves. The CIZA J2242.8+5301 ('sausage') and 1RXS J0603.3+4213 (`toothbrush') clusters ($z\sim 0.2$) host enormous radio-emitting shocks with simple geometry. We investigate the role of mergers and shocks in shaping the H$\alpha$ luminosity function, using custom-made narrow-band filters matching the cluster redshifts mounted on the INT. We surveyed $\sim 0.28$ deg${}^2$ for each cluster and found $181$ line emitters in the `sausage' (volume of $3.371\times 10^3$ Mpc${}^3$ for H$\alpha$ at $z=0.1945$) and $141$ in the `toothbrush' ($4.546\times 10^3$ Mpc${}^3$ for H$\alpha$ at $z=0.225$), out of which $49$ (`sausage') and $30$ (`toothbrush') are expected to be H$\alpha$. We build luminosity functions for the field-of-view down to an average limiting star formation rate of $0.14$ M${}_{\odot }$ yr${}^{-1}$, find good agreement with field luminosity functions at $z=0.2$, but significant differences between the shapes of the luminosity functions for the two clusters. We discover extended, tens-of-kpc-wide H$\alpha$ haloes in galaxies neighbouring relics, which were possibly disrupted by the passage of the shock wave. By comparing the `sausage' cluster with blank fields and other clusters, we also uncover an order of magnitude boost (at $9\sigma$ level) in the normalisation ${\varphi }^{\ast }$ of the luminosity function in the relic areas. Our results suggest that cluster mergers may play an important role in the evolution of cluster galaxies through shock-induced star formation.

Accepted for publication in MNRAS, 14 pages, 9 figures

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