- Abstract:
-
A semi-analytic model of cluster cooling flows is presented. The model assumes that episodic nuclear activity followed by radiative cooling without mass-dropout cycles the cluster gas between a relatively homogeneous, nearly isothermal post-outburst state and a cuspy configuration in which a cooling catastrophe initiates the next nuclear outburst. Fitting the model to Chandra data for the Hydra cluster, a lower limit of $284\Myr$ until the next outburst of Hydra A is derived. Density, tempera...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1046/j.1365-8711.2003.06131.x
-
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- Journal:
- MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
- Volume:
- 338
- Issue:
- 4
- Pages:
- 837-845
- Publication date:
- 2002-07-04
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- URN:
-
uuid:a2a6654c-1471-4b36-8e37-b0b84724fa0b
- Source identifiers:
-
16733
- Local pid:
- pubs:16733
- Language:
- English
- Keywords:
- Copyright date:
- 2002
- Notes:
-
Accepted for publication by MNRAS, revised version to fit published
version, now includes discussion of power-law mass distribution
Journal article
Simple models of cooling flows
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