Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S342(14), p. 133-136, 2018

DOI: 10.1017/s1743921318005185

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Close-up view of an ongoing merger between the NGC 4839 group and the Coma cluster

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

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Preprint: archiving allowed
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Postprint: archiving allowed
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Published version: archiving forbidden
Data provided by SHERPA/RoMEO

Abstract

AbstractWe analyse archival XMM-Newton observations of the massive galaxy group NGC 4839 falling into the Coma cluster core, which reveal a complex morphology for the merger. By comparing high quality X-ray maps of the merging subcluster with SPH simulations, we propose an infall scenario which qualitatively reproduces the observed structure of the NGC 4839 tail.

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