Discovery of a Galaxy Cluster Merger in Unexplored Merger Phase-space

Astronomy and Astrophysics – Astronomy

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Scientific paper

We present DLSCL J1916.2+2951 (z=0.53), a newly discovered major cluster merger in which the collisional cluster gas has become separated from the collisionless galaxies and dark matter. Our identification of the system as a dissociative merger using only optical, weak-lensing, and Sunyaev-Zel'dovich effect observations shows that these systems can be found independently of X-ray observations. We confirm the post-merger scenario using follow-up observations with Keck, Subaru, Hubble Space Telescope, and Chandra, and constrain the dark matter self-interaction cross-section σDMmDM-1ɟ cm2g-1. The system is observed at least 0.7±0.2 Gyr since first pass-through, thus providing a picture of cluster mergers 2-5 times further progressed than similar systems observed to date. This improved temporal leverage has implications for our understanding of merging clusters and their impact on galaxy evolution.

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