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Quantifying properties of ICM inhomogeneities
I. Zhuravleva, E. Churazov, A. Kravtsov +3
We present a new method to identify and characterize the structure of the intracluster medium (ICM) in simulated galaxy clusters. The method uses the median of gas properties, such…
Planck intermediate results. VIII. Filaments between interacting clusters
Planck Collaboration, P. A. R. Ade, N. Aghanim +208
About half of the baryons of the Universe are expected to be in the form of filaments of hot and low density intergalactic medium. Most of these baryons remain undetected even by t…
X-ray emission from star-forming galaxies - II. Hot interstellar medium
S. Mineo, M. Gilfanov, R. Sunyaev
We study the emission from the hot interstellar medium in a sample of nearby late type galaxies defined in Paper I. Our sample covers a broad range of star formation rates, from ~0…
Constraints on the ICM velocity power spectrum from the X-ray lines width and shift
I. Zhuravleva, E. Churazov, A. Kravtsov +1
Future X-ray observations of galaxy clusters by high spectral resolution missions will provide spatially resolved measurements of the energy and width for the brightest emission li…