A parametric physical model for the intracluster medium and its use in joint SZ/X-ray analyses of galaxy clusters
We present a parameterized model of the intra-cluster medium that is suitable for jointly analysing pointed observations of the Sunyaev-Zel'dovich (SZ) effect and X-ray emission in galaxy clusters. The model is based on assumptions of hydrostatic equilibrium, the Navarro, Frenk and White (NFW)...
المؤلفون الرئيسيون: | Allison, JR, Taylor, A, Jones, M, Rawlings, S, Kay, S |
---|---|
التنسيق: | Journal article |
اللغة: | English |
منشور في: |
2010
|
مواد مشابهة
-
GALAXY CLUSTERS IN THE SWIFT /BURST ALERT TELESCOPE ERA: HARD X-RAYS IN THE INTRACLUSTER MEDIUM
حسب: Ajello, M., وآخرون
منشور في: (2015) -
Radio galaxies and energetics of the intracluster medium
حسب: Begelman, M
منشور في: (2002) -
The properties of the X-ray holes in the intracluster medium of the
Perseus cluster
حسب: Fabian, A, وآخرون
منشور في: (2001) -
Generation of internal waves by buoyant bubbles in galaxy clusters and heating of intracluster medium
حسب: Zhang, C, وآخرون
منشور في: (2018) -
A joint SZ–X-ray–optical analysis of the dynamical state of 288 massive galaxy clusters
منشور في: (2021)