A. Stroe, T. Oosterloo, H. J. A. Röttgering, D. Sobral, R. J. van Weeren, W. A. Dawson

Abstract
CIZA J2242.8+5301 (z = 0.188, nicknamed ‘Sausage’) is an extremely massive (M₂₀₀ ∼ 2.0 × 10¹⁵ M_⊙), merging cluster with shock waves towards its outskirts, which was found to host numerous emission line galaxies. We performed extremely deep Westerbork Synthesis Radio Telescope H i observations of the ‘Sausage’ cluster to investigate the effect of the merger and the shocks on the gas reservoirs fuelling present and future star formation (SF) in cluster members. By using spectral stacking, we find that the emission line galaxies in the ‘Sausage’ cluster have, on average, as much H i gas as field galaxies (when accounting for the fact cluster galaxies are more massive than the field galaxies), contrary to previous studies. Since the cluster galaxies are more massive than the field spirals, they may have been able to retain their gas during the cluster merger. The large H i reservoirs are expected to be consumed within ∼0.75–1.0 Gyr by the vigorous SF and active galactic nuclei activity and/or driven out by the outflows we observe. We find that the star formation rate (SFR) in a large fraction of H α emission line cluster galaxies correlates well with the radio broad-band emission, tracing supernova remnant emission. This suggests that the cluster galaxies, all located in post-shock regions, may have been undergoing sustained SFR for at least 100 Myr. This fully supports the interpretation proposed by Stroe et al. and Sobral et al. that gas-rich cluster galaxies have been triggered to form stars by the passage of the shock.

Keywords
shock waves - galaxies: active - galaxies: clusters: individual: CIZA J2242.8+5301 - radio continuum: galaxies - radio lines: galaxies

Monthly Notices of the Royal Astronomical Society
Volume 452, Issue 3, Page 2731
2015 September

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