The evolution of classical double radio galaxies
Being immensely powerful, and hence detectable out to great distances, classical double radio galaxies have long been recognised as cosmological probes of great potential. Before this potential can be realised, it is necessary to understand the physical mechanisms by which these objects evolve and c...
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| Μορφή: | Conference item |
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2002
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| _version_ | 1826298239146524672 |
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| author | Blundell, K |
| author_facet | Blundell, K |
| author_sort | Blundell, K |
| collection | OXFORD |
| description | Being immensely powerful, and hence detectable out to great distances, classical double radio galaxies have long been recognised as cosmological probes of great potential. Before this potential can be realised, it is necessary to understand the physical mechanisms by which these objects evolve and change with time. This chapter describes how to deduce from classical double radio source observables (luminosity, spectral index, redshift and linear size) the essential nature of how these objects evolve and the true relationships between the underlying physical parameters (jet-power, age etc). I discuss the key role played by hotspots in governing the energy distribution of the lobes they feed, and subsequent spectral evolution. |
| first_indexed | 2024-03-07T04:43:49Z |
| format | Conference item |
| id | oxford-uuid:d2919b51-51a5-4aa3-b6f3-6a80e0d9f4b9 |
| institution | University of Oxford |
| last_indexed | 2024-03-07T04:43:49Z |
| publishDate | 2002 |
| record_format | dspace |
| spelling | oxford-uuid:d2919b51-51a5-4aa3-b6f3-6a80e0d9f4b92022-03-27T08:04:49ZThe evolution of classical double radio galaxiesConference itemhttp://purl.org/coar/resource_type/c_5794uuid:d2919b51-51a5-4aa3-b6f3-6a80e0d9f4b9Symplectic Elements at Oxford2002Blundell, KBeing immensely powerful, and hence detectable out to great distances, classical double radio galaxies have long been recognised as cosmological probes of great potential. Before this potential can be realised, it is necessary to understand the physical mechanisms by which these objects evolve and change with time. This chapter describes how to deduce from classical double radio source observables (luminosity, spectral index, redshift and linear size) the essential nature of how these objects evolve and the true relationships between the underlying physical parameters (jet-power, age etc). I discuss the key role played by hotspots in governing the energy distribution of the lobes they feed, and subsequent spectral evolution. |
| spellingShingle | Blundell, K The evolution of classical double radio galaxies |
| title | The evolution of classical double radio galaxies |
| title_full | The evolution of classical double radio galaxies |
| title_fullStr | The evolution of classical double radio galaxies |
| title_full_unstemmed | The evolution of classical double radio galaxies |
| title_short | The evolution of classical double radio galaxies |
| title_sort | evolution of classical double radio galaxies |
| work_keys_str_mv | AT blundellk theevolutionofclassicaldoubleradiogalaxies AT blundellk evolutionofclassicaldoubleradiogalaxies |