Results 41 to 50 of about 2,319,978 (287)
On the helium fingers in the intracluster medium [PDF]
Monthly Notices of the Royal Astronomical Society, 2017 7 pages, 1 ...
Sagar Chakraborty +2 more
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Universal thermodynamic properties of the intracluster medium over two decades in radius in the X-COP sample [PDF]
Astronomy & Astrophysics, 2018 Context. The hot plasma in a galaxy cluster is expected to be heated to high temperatures through shocks and adiabatic compression. The thermodynamical properties of the gas encode information on the processes leading to the thermalization of the gas in ...
V. Ghirardini +12 more
semanticscholar +1 more source
Cosmological simulations of the intracluster medium [PDF]
Monthly Notices of the Royal Astronomical Society, 2004 We investigate the properties of the intracluster medium (ICM) that forms within N-body/hydrodynamical simulations of galaxy clusters in a \LambdaCDM cosmology. When radiative cooling and a simple model for galactic feedback are included, our clusters have X-ray luminosities and temperatures in good agreement with observed systems, demonstrating the ...
Adrian Jenkins +3 more
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Heating and enriching the intracluster medium [PDF]
Monthly Notices of the Royal Astronomical Society, 2012 23 pages, accepted by MNRAS. Some changes in response to referee's comments.
Owain Young +2 more
openaire +3 more sources
Electron Reacceleration via Ion Cyclotron Waves in the Intracluster Medium
The Astrophysical Journal, 2023 In galaxy clusters, the intracluster medium (ICM) is expected to host a diffuse, long-lived, and invisible population of “fossil” cosmic-ray electrons (CRe) with 1–100 MeV energies.
Aaron Tran +4 more
doaj +1 more source
Formation of multiphase plasma in galactic haloes and an analogy to solar plasma
Frontiers in Astronomy and Space Sciences, 2023 Thermal instability (TI) potentially explains the origin of cold gas in the intracluster medium (ICM), which is heated sufficiently by AGN feedback. The Hα filaments seen in cluster cores provide strong motivation for TI.
Prakriti Pal Choudhury
doaj +1 more source
The loss of the intracluster medium in globular clusters [PDF]
, 2020 Stars in globular clusters (GCs) lose a non negligible amount of mass during their post-main sequence evolution. This material is then expected to build up a substantial intra-cluster medium (ICM) within the GC.
W. Chantereau +5 more
semanticscholar +1 more source
Calcium-rich Gap Transients: Solving the Calcium Conundrum in the Intracluster Medium [PDF]
, 2014 X-ray measurements suggest the abundance of Calcium in the intracluster medium is higher than can be explained using favored models for core-collapse and Type Ia supernovae alone.
Kasliwal, Mansi M. +2 more
core +2 more sources
Dynamical evolution of magnetic fields in the intracluster medium [PDF]
Monthly notices of the Royal Astronomical Society, 2019 We investigate the evolution of magnetic fields in galaxy clusters starting from constant primordial fields using highly resolved ($\approx \rm 4 ~kpc$) cosmological MHD simulations.
P. Dom'inguez-Fern'andez +3 more
semanticscholar +1 more source
The Magnetothermal Instability in the Intracluster Medium [PDF]
The Astrophysical Journal, 2008 The electron mean free path in the intracluster medium (ICM) of galaxy clusters is much larger than the gyroradius; thus, heat is transported anisotropically along magnetic field lines. We show that the intracluster medium is unstable to the magnetothermal instability (MTI) using MHD simulations with anisotropic thermal conduction.
James M. Stone +3 more
openaire +4 more sources