Decoding X-ray observations from centres of galaxy clusters using MCMC
arXiv:1601.02347 · doi:10.1093/mnras/stw1062
Abstract
We correct for the use of electron densities instead of total gas density in the pressure fits which were used to derive the local free-fall times (t) in the original paper.
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- The inner gas mass-temperature profile in the core of nearby galaxy clusters