English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

Multi-wavelength techniques can probe the distribution and the physicalproperties of baryons and dark matter in galaxy clusters from the inner regionsout to the peripheries. We present a full three-dimensional analysis combiningstrong and weak lensing, X-ray surface brightness and temperature, and theSunyaev-Zel'dovich effect. The method is applied to MACS J1206.2-0847, aremarkably regular, face-on, massive, M_{200}=(1.1+-0.2)*10^{15}M_Sun/h,cluster at z=0.44. The measured concentration, c_{200}=6.3+-1.2, and thetriaxial shape are common to halos formed in a LCDM scenario. The gas hassettled in and follows the shape of the gravitational potential, which isevidence of pressure equilibrium via the shape theorem. There is no evidencefor significant non-thermal pressure and the equilibrium is hydrostatic.

CLUMP-3D. Three dimensional lensing and multi-probe analysis of MACS J1206.2-0847, a remarkably regular cluster