Results 31 to 40 of about 16,927 (234)
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
The nature of the motions of multiphase filaments in the centers of galaxy clusters
Frontiers in Astronomy and Space Sciences, 2023 The intracluster medium (ICM) in the centers of galaxy clusters is heavily influenced by the “feedback” from supermassive black holes (SMBHs). Feedback can drive turbulence in the ICM and turbulent dissipation can potentially be an important source of ...
Shalini Ganguly +9 more
doaj +1 more source
Coulomb interactions in the intracluster medium [PDF]
Monthly Notices of the Royal Astronomical Society, 1998 4 pages, accepted as a Letter in the ...
Stefano Ettori, Andrew C. Fabian
openaire +4 more sources
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
Modelling the Energy Spectra of Radio Relics
Galaxies, 2021 Radio relics are diffuse synchrotron sources that illuminate shock waves in the intracluster medium. In recent years, radio telescopes have provided detailed observations about relics.
Denis Wittor +2 more
doaj +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
Chemical Evolution of Galaxies and Intracluster Medium [PDF]
, 2002 In this series of lectures I discuss the basic principles and the modelling of the chemical evolution of galaxies. In particular, I present models for the chemical evolution of the Milky Way galaxy and compare them with the available observational data.
F. Matteuccí
openalex +4 more sources
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
Mapping the intracluster medium temperature in the era of NIKA2 and MUSTANG-2 [PDF]
EPJ Web of Conferences, 2022 We present preliminary results from an on-going program that aims at mapping the intracluster medium (ICM) temperature of high redshift galaxy clusters from the MaDCoWS sample using a joint analysis of shallow X-ray data obtained by Chandra and high ...
Ruppin F. +52 more
doaj +1 more source
Intracluster Medium through three years of WMAP [PDF]
, 2006 Wilkinson Microwave Anisotropy Probe (WMAP) has provided us with the yet highest resolution all-sky maps of the Cosmic Microwave Background. As a result of thermal Sunyaev-Zel'dovich effect, clusters of galaxies are imprinted as tiny, poorly resolved ...
Afshordi +22 more
core +3 more sources