Artigo Acesso aberto Revisado por pares

A mosaic of the Coma cluster of galaxies with XMM-Newton

2001; EDP Sciences; Volume: 365; Issue: 1 Linguagem: Inglês

10.1051/0004-6361

ISSN

1432-0746

Autores

U. G. Briel, J. P. Henry, David H. Lumb, M. Arnaud, D. M. Neumann, N. Aghanim, R. Gastaud, J. P. D. Mittaz, T. P. Sasseen, W. T. Vestrand,

Tópico(s)

Pulsars and Gravitational Waves Research

Resumo

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.

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