Cluster Shock Waves
Cluster Shock Waves is a physical phenomenon in astrophysics denoting a propagating discontinuity in the intracluster medium of galaxy clusters, characterized by a sudden increase in gas density, temperature, and pressure due to supersonic flow driven by gravitational structure formation or mergers.
377
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26.4K
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920
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454
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Publications per year
2017–2026
69
Variants
Intracluster Shock Waves
Parents
377
Shocks and cold fronts in galaxy clusters
Maxim Markevitch, A. Vikhlinin · Physics Reports · 2007 · 747 citations · Full text
Natural Sciences, Astronomy, Physics +10
High-energy ions produced in explosions of superheated atomic clusters
J. W. G. Tisch, Emma Springate, M. B. Mason et al. · Nature · 1997 · 626 citations
A Textbook Example of a Bow Shock in the Merging Galaxy Cluster 1E 0657-56
Maxim Markevitch, Anthony H. Gonzalez, L. P. David et al. · The Astrophysical Journal · 2002 · 624 citations · Full text
Natural Sciences, Astronomy, Physics +13
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Center for Astrophysics Harvard & Smithsonian, United States
15 publications · 1.1K citations
15
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1–5 of 920
454
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
34 h-index
142 publications
14.8K citations
Leiden University
Leiden, The Netherlands
29 h-index
104 publications
7K citations
Istituto di Radioastronomia di Bologna
Bologna, Italy
27 h-index
98 publications
7.7K citations
Universität Hamburg
Hamburg, Germany
22 h-index
69 publications
4.5K citations
Max Planck Institute for Astrophysics
Garching, Germany
21 h-index
38 publications
2.6K citations

Imperial College London
London, United Kingdom
20 h-index
71 publications
7.5K citations

University of Bologna
Bologna, Italy
20 h-index
48 publications
3.4K citations
Thüringer Landessternwarte Tautenburg
Tautenburg, Germany
18 h-index
21 publications
1.7K citations
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ApJ · 79 publications · 5.8K citations
45
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72 publications · 6.5K citations
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18 publications · 1.1K citations
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11 publications · 511 citations
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Repository · 10 publications · 496 citations
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