The heating of gas in a galaxy cluster by X-ray cavities and large-scale shock fronts
Nulsen, P. E. J. ; Wise, M. W. ; Rafferty, D. A. ; Carilli, C. ; Sarazin, C. L. ; Blanton, E. L. ; McNamara, B. R.
[s.l.] : Macmillian Magazines Ltd.
Published 2005
[s.l.] : Macmillian Magazines Ltd.
Published 2005
| ISSN: |
1476-4687
|
|---|---|
| Source: |
Nature Archives 1869 - 2009
|
| Topics: |
Biology
Chemistry and Pharmacology
Medicine
Natural Sciences in General
Physics
|
| Notes: |
[Auszug] Most of the baryons in galaxy clusters reside between the galaxies in a hot, tenuous gas. The densest gas in their centres should cool and accrete onto giant central galaxies at rates of 10–1,000 solar masses per year. No viable repository for this gas, such as clouds or new stars, ...
|
| Type of Medium: |
Electronic Resource
|
| URL: |