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X-raying galaxies: a Chandra legacy. [PDF]
Wang QD.
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Cosmology and Fundamental Physics with the Euclid Satellite. [PDF]
Amendola L +63 more
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Chandra enables study of x-ray jets. [PDF]
Schwartz D.
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Real or virtual large-scale structure? [PDF]
Evrard AE.
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A multi-wavelength study of the intracluster medium in the galaxy clusters
2023Galaxy clusters consist of galaxies, dark matter, and extremely hot electron gas also known as intra-cluster medium (ICM). The ICM can influence galaxy evolution by interacting with the galaxy via ram pressure stripping or cutting off the gas supply of the galaxy.
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1984
Analyses of the x-ray images obtained with the Einstein Observatory have provided a new and different view of clusters of galaxies. The primary topics discussed in this review are the role of the central dominant galaxy, the origin of SO galaxies, cluster classification and the dynamically young state of most clusters, the large scale height of the gas
C. Jones, W. Forman
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Analyses of the x-ray images obtained with the Einstein Observatory have provided a new and different view of clusters of galaxies. The primary topics discussed in this review are the role of the central dominant galaxy, the origin of SO galaxies, cluster classification and the dynamically young state of most clusters, the large scale height of the gas
C. Jones, W. Forman
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SUPPRESSION OF ELECTRON THERMAL CONDUCTION IN THE HIGH β INTRACLUSTER MEDIUM OF GALAXY CLUSTERS
2019Understanding the thermodynamic state of the hot intracluster medium (ICM) in a galaxy cluster requires a 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.
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