- Abstract:
-
Active galactic nuclei are clearly heating gas in `cooling flows'. The effectiveness and spatial distribution of the heating are controversial. We use three-dimensional simulations on adaptive grids to study the impact on a cooling flow of weak, subrelativistic jets. The simulations show cavities and vortex rings as in the observations. The cavities are fast-expanding dynamical objects rather than buoyant bubbles as previously modelled, but shocks still remain extremely hard to detect with X-...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1111/j.1365-2966.2004.07382.x
-
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- Journal:
- Mon.Not.Roy.Astron.Soc.
- Volume:
- 348
- Issue:
- 4
- Pages:
- 1105
- Publication date:
- 2003-07-27
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- URN:
-
uuid:6eda5852-459a-4477-931c-2df073b4f846
- Source identifiers:
-
167463
- Local pid:
- pubs:167463
- Language:
- English
- Keywords:
- Copyright date:
- 2003
- Notes:
-
16 pages, 15 figures. Accepted for publication in MNRAS. Revised
version taking referee's comments into account, minor changes.
High-resolution version and MPEGs can be found at
http://www.clusterheating.org/papers.php
Journal article
Heating cooling flows with jets
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