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2008MNRAS.386..278G - Mon. Not. R. Astron. Soc., 386, 278-288 (2008/May-1)
The weak shock in the core of the Perseus cluster.
GRAHAM J., FABIAN A.C. and SANDERS J.S.
Abstract (from CDS):
We also calculate the thermal energy liberated by the weak shock. The total energy in the shocked region is about 3.5 times the work needed to inflate the bubbles adiabatically, and the power of the shock is around 6x1044/ergs per bubble, just over 1045/ergs in total.
Abstract Copyright: ©2008 The Authors. Journal compilation © 2008 RAS
Journal keyword(s): clusters: individual: Perseus - cooling flows - intergalactic medium - X-rays: galaxies - galaxies
Simbad objects: 4
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