SUPPRESSION OF ELECTRON THERMAL CONDUCTION IN THE HIGH β INTRACLUSTER MEDIUM OF GALAXY CLUSTERS [PDF]
The Astrophysical Journal Letters, 2016 ABSTRACT Understanding the thermodynamic state of the hot intracluster medium (ICM) in a galaxy cluster requires knowledge of the plasma transport processes, especially thermal conduction. The basic physics of thermal conduction in plasmas with ICM-like conditions has yet to be elucidated, however. We use particle-in-cell simulations and
Roberg-Clark, GT +3 more
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A Comparison of the Galaxy Populations in the Coma and Distant Clusters: The Evolution of k+a Galaxies and the Role of the Intracluster Medium [PDF]
The Astrophysical Journal, 2004 21 pages, 7 figures, to appear in ApJ, version after referee's ...
Poggianti, B. M. +7 more
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Uncertainty in Mass Determination of Galaxy Clusters due to the Bulk Motion of Intracluster Medium [PDF]
Symposium - International Astronomical Union, 1998 Determination of the mass of cluster of galaxies (CG) is very important mainly because it relates to determination of cosmological density parameter (Ω0).
M. Takizawa, S. Mineshige
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Generation of internal waves by buoyant bubbles in galaxy clusters and heating of intracluster medium [PDF]
Monthly Notices of the Royal Astronomical Society, 2018 15 pages, 13 figures, submitted to ...
Zhang, C, Churazov, E, Schekochihin, A
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The XMM Cluster Survey: The interplay between the brightest cluster galaxy and the intra-cluster medium via AGN feedback [PDF]
Royal Astronomical Society. Monthly Notices, 2012 Accepted for publication in MNRAS - replaced to match corrected ...
Stott, John P. +18 more
+9 more sources
Two‐Phase Intracluster Medium in the Centaurus Cluster of Galaxies
The Astrophysical Journal, 1999 accepted for publication in ...
Ikebe, Yasushi +6 more
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On the origin of central abundance drops in the intracluster medium of galaxy groups and clusters [PDF]
Monthly Notices of the Royal Astronomical Society, 2019 A central drop of ICM Fe abundance has been observed in several cool-core clusters. It has been proposed that this abundance drop may be due, at least partially, to the depletion of Fe into dust grains in the central, high-density regions. According to this scenario, noble gas elements such as Ar and Ne are not expected to be depleted into dust, and ...
Ang Liu, Meng Zhai, Paolo Tozzi
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The Multiphase Nature of the Intracluster Medium of Some Clusters of Galaxies
The Astrophysical Journal, 2001 ApJ ...
Bonamente, Massimiliano +2 more
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Galaxy Evolution in a Pilot Survey up to z = 1 and CDM Halos
Advances in Astronomy, Volume 2011, Issue 1, 2011., 2011 We study spectral evolution of galaxies in a magnitude limited sample of 550 galaxies from z = 1 down to z = 0.3 on a pencil beam of ≈10′ × 10′. We concentrate on the large apparent cosmological structures along the line of sight, and we bin our individual galaxy spectra to obtain representative high S/N spectra based upon these structures.
E. Giraud +7 more
wiley +1 more source
Advances in Astronomy, Volume 2011, Issue 1, 2011., 2011 Dark matter is one of the greatest unsolved mysteries in cosmology at the present time. About 80% of the Universe′s gravitating matter is nonluminous, and its nature and distribution are for the most part unknown. In this paper, we will outline the history, astrophysical evidence, candidates, and detection methods of dark matter, with the goal to give ...
Katherine Garrett +2 more
wiley +1 more source