A study of diffusive shock acceleration as a process explaining observations of 1 E0657-56 galaxy cluster

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dc.creatorSiemieniec-Ozieblo, G.
dc.date2004-04-20
dc.date.accessioned2026-07-07T02:12:56Z
dc.date.available2026-07-07T02:12:56Z
dc.descriptionChandra X-ray observations of the 1 E0657-56 galaxy cluster diffuse emission reveal the existence of large scale cluster merger shock. We study the observed radio and X-ray data of this cluster as a possible result of the diffusive shock acceleration. This model can explain the observations within reasonable ranges of physical parameters for the shock and the intracluster medium. The expected nonthermal soft and hard X-ray fluxes are predicted.
dc.description9 pages, accepted for Acta Phys. Polon.B
dc.identifierhttps://arxiv.org/abs/astro-ph/0404375
dc.identifierhttp://arxiv.org/abs/astro-ph/0404375
dc.identifierActa Phys.Polon. B35 (2004) 2131-2140
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7636
dc.subjectAstrophysics
dc.titleA study of diffusive shock acceleration as a process explaining observations of 1 E0657-56 galaxy cluster
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