pith. sign in

arxiv: astro-ph/0012215 · v1 · submitted 2000-12-11 · 🌌 astro-ph

Temperature Structure of Four Merging Clusters Obtained with Chandra

classification 🌌 astro-ph
keywords temperaturea2163a665a754a2218chandraclusterclusters
0
0 comments X
read the original abstract

We present preliminary Chandra results on z=0.2 clusters A665, A2163 and A2218, and a z=0.05 cluster A754. For A754, A665 and A2163, we have derived first high-resolution projected gas temperature maps. All three show strong spatial temperature variations in the inner r<0.5-1 Mpc regions, indicating ongoing mergers. The maps reveal a probable shock in front of a moving cluster core in A665, a rather complicated temperature distribution in the center of A2163, and possibly a merger of three subclusters in A754. At greater off-center distances, radial profiles for A2163 and A2218 show a temperature decline, in agreement with earlier ASCA results.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.