Temperature Map and Iron Abundance of the Ophiuchus Cluster of Galaxies

Astronomy and Astrophysics – Astronomy

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Galaxies: Clusters: Individual (Ophiuchus), Galaxies: Evolution, X-Rays: Galaxies

Scientific paper

We present an X-ray surface-brightness distribution and a temperature map of the Ophiuchus cluster of galaxies observed by ASCA. The Ophiuchus cluster is a nearby rich cluster located at z=0.028 having an angular extent of ~1°. The observations were made by five pointings that cover the whole cluster. After deconvolution with the ASCA complex response function, we obtained the surface-brightness distribution with an angular resolution of 2' and a temperature map with 8' resolution. The X-ray surface-brightness distribution shows a nearly spherically symmetric distribution, except for a 15σ image excess at the position of 10' to the north of the cluster center. On the other hand, a hot region with a temperature > 13 keV is spread over a region of 20' × 30' at 20' to the west of the cluster center. Because these characteristics are similar to those of the Coma cluster, we conclude this cluster has never relaxed dynamically, and is also recently experienced a merger.

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