The DOI matches its Crossref record; 12 of the 12 references it cites were found in a registry or an index.
Reviving fossil radio plasma in clusters of galaxies by adiabatic compression in environmental shock waves
Open accessAbstract
We give for a plasma with a history of several expansion and contraction phases an analytical model of the evolution of a contained relativistic electron population under synchrotron, inverse Compton and adiabatic energy losses or gains. This is applied to different scenarios for evolution of radio plasma inside the cocoons of radio galaxies, after the activity of the central engine has ceased. It is demonstrated that fossil radio plasma with an age of even up to 2 Gyr can be revived by compression in a shock wave of large-scale structure formation, caused during the merging events of galaxy clusters, or by the accretion onto galaxy clusters. We argue, that this is a highly plausible explanation for the observed cluster radio relics, which are the regions of diffuse radio emission found in clusters of galaxies, without any likely parent radio galaxy seen nearby. An implication of this model is the existence of a population of diffuse, ultra-steep spectrum, very low frequency radio sources located inside and possibly outside of clusters of galaxies, tracing the revival of aged fossil radio plasma by the shock waves associated with large-scale structure formation.
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Cites
The Dynamical State of the Interstellar Gas and Field
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Overpressured cocoons in extragalactic radio sources
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A self-similar model for extragalactic radio sources
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A systematic asymmetry in the polarization properties of double radio sources with one jet
Garrington, S. T., Leahy, J. P., Conway, R. G., & Laingt, R. A. (1988) · Nature · doi:10.1038/331147a0 · Cited by 334
Radio halo and relic candidates from the NRAO VLA Sky Survey
Giovannini, G., Tordi, M., & Feretti, L. (1999) · New Astronomy · doi:10.1016/s1384-1076(99)00018-4 · Cited by 317
A model for the magnetic-field structure in extended radio sources
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Properties of Cosmic Shock Waves in Large‐Scale Structure Formation
Miniati, F., Ryu, D., Kang, H., Jones, T. W., Cen, R., & Ostriker, J. P. (2000) · The Astrophysical Journal · doi:10.1086/317027 · Cited by 280
A Cluster Merger and the Origin of the Extended Radio Emission in Abell 3667
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The extended radio emission in the luminous X-ray cluster A3667
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Cited by
Shocks and cold fronts in galaxy clusters
Markevitch, M., & Vikhlinin, A. (2007) · Physics Reports · doi:10.1016/j.physrep.2007.01.001 · Cited by 726
Carilli, C. L., & Taylor, G. B. (2002) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.40.060401.093852 · Cited by 709
Clusters of galaxies: observational properties of the diffuse radio emission
Feretti, L., Giovannini, G., Govoni, F., & Murgia, M. (2012) · The Astronomy and Astrophysics Review · doi:10.1007/s00159-012-0054-z · Cited by 667
COSMIC RAYS IN GALAXY CLUSTERS AND THEIR NONTHERMAL EMISSION
BRUNETTI, G., & JONES, T. W. (2014) · International Journal of Modern Physics D · doi:10.1142/s0218271814300079 · Cited by 577
Diffuse Radio Emission from Galaxy Clusters
van Weeren, R. J., de Gasperin, F., Akamatsu, H., Brüggen, M., Feretti, L., Kang, H., Stroe, A., & Zandanel, F. (2019) · Space Science Reviews · doi:10.1007/s11214-019-0584-z · Cited by 481
Metadata
- Authors
- Enßlin, T. A., & Gopal-Krishna
- Venue
- Astronomy & Astrophysics
- Publisher
- EDP Sciences
- Published
- 2001-01
- Volume
- 366
- Issue
- 1
- Pages
- 26-34
- ISSN
- 0004-6361 (ISSN-L)
- 1432-0746
- OpenAlex
- W2065839045
- Cited by
- 273
- References
- 12
- FWCI
- 6.63
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Enßlin, T. A., & Gopal-Krishna. (2001). Reviving fossil radio plasma in clusters of galaxies by adiabatic compression in environmental shock waves. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361%3A20000198
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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