pith. sign in

arxiv: astro-ph/0011323 · v1 · submitted 2000-11-16 · 🌌 astro-ph

A Mosaic of the Coma Cluster of Galaxies with XMM-Newton

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

The Coma cluster of galaxies was observed with XMM-Newton in 12 partially overlapping pointings. We present here the resulting X-ray map in different energy bands and discuss the large scale structure of this cluster. Many point sources were found throughout the observed area, at least 11 of them are coincident with bright galaxies. We also give a hardness ratio map at the so far highest angular resolution obtained for a cluster of galaxies. In this map we found soft regions at the position of bright galaxies, little variation in the central 15 arcmin, but some harder regions north of the line NGC 4874 - NGC 4889.

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.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Introduction to multi-messenger astronomy

    astro-ph.HE 2019-07 unverdicted

    The paper supplies an introductory lecture-style summary of observational techniques, astronomical sources, and physical processes across the four main messengers in multi-messenger astronomy.