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A Distant Chandra Galaxy Cluster CL J1415.1+3612: Constraint on Evidence of the Cool-Core Phenomenon
2014
Open Astronomy
Deep Chandra observations of the distant cluster of galaxies, CL J1415.1+3612, are analyzed in order to determine the main physical characteristics of the intracluster medium. We also investigate some properties of a cool-core phenomenon at ∼ 10 kpc. Combining all Chandra observations, we derive the average temperature (kT = 6.77±0.54 keV) and the metal abundance (Z = 0.84±0.16 Z ⊙ ) of the cluster. Assuming hydrostatic equilibrium and spherical symmetry, and using deprojected temperature and
doi:10.1515/astro-2017-0174
fatcat:y62qloqer5asthe277l7tyw2e4