The hydrodynamics of radio galaxy cocoons
We use numerical simulations to discuss some aspects of the hydrodynamics of radio galaxies, and the affect that hydrodynamical considerations have on the long term evolution of such sources. Using these simulations, we can start to assess the impact that a radio galaxy may have on the energy and en...
Main Author: | |
---|---|
Format: | Conference item |
Published: |
2002
|
_version_ | 1797094105659998208 |
---|---|
author | Reynolds, C |
author_facet | Reynolds, C |
author_sort | Reynolds, C |
collection | OXFORD |
description | We use numerical simulations to discuss some aspects of the hydrodynamics of radio galaxies, and the affect that hydrodynamical considerations have on the long term evolution of such sources. Using these simulations, we can start to assess the impact that a radio galaxy may have on the energy and entropy budget of its host galaxy or cluster. A full hydrodynamic treatment of radio galaxy expansion is also necessary to interpret correctly the X-ray shells and cavities that, are seen in some sources by ROSAT and Chandra. |
first_indexed | 2024-03-07T04:09:31Z |
format | Conference item |
id | oxford-uuid:c75936d4-1adf-4164-bf6d-ecde2825ea28 |
institution | University of Oxford |
last_indexed | 2024-03-07T04:09:31Z |
publishDate | 2002 |
record_format | dspace |
spelling | oxford-uuid:c75936d4-1adf-4164-bf6d-ecde2825ea282022-03-27T06:44:25ZThe hydrodynamics of radio galaxy cocoonsConference itemhttp://purl.org/coar/resource_type/c_5794uuid:c75936d4-1adf-4164-bf6d-ecde2825ea28Symplectic Elements at Oxford2002Reynolds, CWe use numerical simulations to discuss some aspects of the hydrodynamics of radio galaxies, and the affect that hydrodynamical considerations have on the long term evolution of such sources. Using these simulations, we can start to assess the impact that a radio galaxy may have on the energy and entropy budget of its host galaxy or cluster. A full hydrodynamic treatment of radio galaxy expansion is also necessary to interpret correctly the X-ray shells and cavities that, are seen in some sources by ROSAT and Chandra. |
spellingShingle | Reynolds, C The hydrodynamics of radio galaxy cocoons |
title | The hydrodynamics of radio galaxy cocoons |
title_full | The hydrodynamics of radio galaxy cocoons |
title_fullStr | The hydrodynamics of radio galaxy cocoons |
title_full_unstemmed | The hydrodynamics of radio galaxy cocoons |
title_short | The hydrodynamics of radio galaxy cocoons |
title_sort | hydrodynamics of radio galaxy cocoons |
work_keys_str_mv | AT reynoldsc thehydrodynamicsofradiogalaxycocoons AT reynoldsc hydrodynamicsofradiogalaxycocoons |