Modelling shock heating in cluster mergers – I. Moving beyond the spherical accretion model
about
Enriching the hot circumgalactic mediumCluster Physics with Merging Galaxy ClustersGas expulsion by quasar-driven winds as a solution to the overcooling problem in galaxy groups and clustersAccretion shocks and cold filaments in galaxy formationRam pressure stripping the hot gaseous haloes of galaxies in groups and clusters
P2860
Modelling shock heating in cluster mergers – I. Moving beyond the spherical accretion model
description
article
@en
im April 2007 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована у квітні 2007
@uk
name
Modelling shock heating in clu ...... the spherical accretion model
@en
Modelling shock heating in clu ...... the spherical accretion model
@nl
type
label
Modelling shock heating in clu ...... the spherical accretion model
@en
Modelling shock heating in clu ...... the spherical accretion model
@nl
prefLabel
Modelling shock heating in clu ...... the spherical accretion model
@en
Modelling shock heating in clu ...... the spherical accretion model
@nl
P2093
P2860
P1476
Modelling shock heating in clu ...... the spherical accretion model
@en
P2093
C. G. Lacey
C. S. Frenk
F. R. Pearce
G. M. Voit
I. G. McCarthy
M. L. Balogh
R. G. Bower
P2860
P304
P356
10.1111/J.1365-2966.2007.11465.X
P407
P577
2007-04-01T00:00:00Z
P818
astro-ph/0701335
P819
2007MNRAS.376..497M