The properties of the X-ray holes in the intracluster medium of the Perseus cluster

Details The properties of the X-ray holes in the intracluster medium of the Perseus cluster The properties of the X-ray holes in the intracluster medium of the Perseus cluster

2001-11-21

arxiv.org/abs/astro-ph/0111418v1

Mon.Not.Roy.Astron.Soc.331:369-375,2002

Astronomy and Astrophysics

Astrophysics

7 pages, accepted for publication in MNRAS

Scientific paper

10.1046/j.1365-8711.2002.05182.x

High resolution X-ray and low frequency radio imaging now allow us to examine in detail the interaction and physical properties of the radio source 3C84 and the surrounding thermal gas. The radiative and dynamical properties of the inner X-ray holes, which coincide with the radio lobes, indicate that the ratio of the energy factor k and filling factor f is in the range 180

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