How do atomic code uncertainties affect abundance measurements in the intracluster medium?
Astronomische Nachrichten, Volume 341, Issue 2, Page 203-209, February 2020., 2020 Abstract Accurate chemical abundance measurements of X‐ray‐emitting atmospheres pervading massive galaxies, galaxy groups, and clusters provide essential information on the star formation and chemical enrichment histories of these large‐scale structures.
François Mernier +8 more
wiley +1 more source
A CHANDRA STUDY OF TEMPERATURE DISTRIBUTIONS OF THE INTRACLUSTER MEDIUM IN 50 GALAXY CLUSTERS [PDF]
The Astrophysical Journal, 2016 ABSTRACT To investigate the spatial distribution of the intracluster medium temperature in galaxy clusters in a quantitative way and probe the physics behind it, we analyze the X-ray spectra from a sample of 50 clusters that were observed with the Chandra ACIS instrument over the past 15 years and measure the radial temperature profiles ...
Zhenghao Zhu +12 more
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The chemical evolution of galaxy clusters: Dissecting the iron mass budget of the intracluster medium [PDF]
Astronomy & Astrophysics, 2020 Aims. We study the chemical evolution of galaxy clusters by measuring the iron mass in the ICM after dissecting the abundance profiles into different components. Methods. We used Chandra archival observations of 186 morphologically regular clusters in the redshift range of [0.04, 1.07].
Liu A. +6 more
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Two‐Temperature Intracluster Medium in Merging Clusters of Galaxies [PDF]
The Astrophysical Journal, 1999 We investigate the evolution of intracluster medium during a cluster merger, explicitly considering the relaxation process between the ions and electrons by N-body and hydrodynamical simulations. When two subclusters collide each other, a bow shock is formed between the centers of two substructures and propagate in both directions along the collision ...
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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
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Dark Matter and Dark Energy Induced by Condensates
Advances in High Energy Physics, Volume 2016, Issue 1, 2016., 2016 It is shown that the vacuum condensate induced by many phenomena behaves as a perfect fluid which, under particular conditions, has zero or negative pressure. In particular, the condensates of thermal states of fields in curved space and of mixed particles have been analyzed.
Antonio Capolupo +1 more
wiley +1 more source