Arithmetic with X-ray images of galaxy clusters: effective equation of state for small-scale perturbations in the ICM
We discuss a novel technique of manipulating X-ray images of galaxy clusters to reveal the nature of small-scale density/temperature perturbations in the intracluster medium (ICM). As we show, this technique can be used to differentiate between sound waves and isobaric perturbations in Chandra image...
Váldodahkkit: | Churazov, E, Arevalo, P, Forman, W, Jones, C, Schekochihin, A, Vikhlinin, A, Zhuravleva, I |
---|---|
Materiálatiipa: | Journal article |
Almmustuhtton: |
Oxford University Press
2016
|
Geahča maid
-
Turbulent heating in galaxy clusters brightest in X-rays.
Dahkki: Zhuravleva, I, et al.
Almmustuhtton: (2014) -
X-ray surface brightness and gas density fluctuations in the Coma cluster
Dahkki: Churazov, E, et al.
Almmustuhtton: (2012) -
The nature and energetics of AGN-driven perturbations in the hot gas in
the Perseus Cluster
Dahkki: Zhuravleva, I, et al.
Almmustuhtton: (2016) -
Physics of cosmic plasmas from high angular resolution X-ray imaging of galaxy clusters
Dahkki: Markevitch, M, et al.
Almmustuhtton: (2019) -
Bubble-driven gas uplift in galaxy clusters and its velocity features
Dahkki: Zhang, C, et al.
Almmustuhtton: (2022)