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

Abstract:
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
Publication status:
Published

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Authors


Fabian, AC More by this author
Celotti, A More by this author
More by this author
Institution:
University of Oxford
Department:
Oxford, MPLS, Physics, Astrophysics
Kassim, NE More by this author
Perley, RA More by this author
Journal:
Mon.Not.Roy.Astron.Soc.
Volume:
331
Issue:
2
Pages:
369-375
Publication date:
2001-11-21
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
URN:
uuid:2912e387-0cad-4747-b532-17997249ef53
Source identifiers:
1725
Local pid:
pubs:1725
Language:
English
Keywords:

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