SHOCK HEATING OF THE MERGING GALAXY CLUSTER A521-Reference-Cited by-同舟云学术

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SHOCK HEATING OF THE MERGING GALAXY CLUSTER A521

Published:2013-01-29 Issue:1 Volume:764 Page:82
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Bourdin H.,Mazzotta P.,Markevitch M.,Giacintucci S.,Brunetti G.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/764/i=1/a=82/pdf

Reference45 articles.

1. Photoelectric absorption cross sections with variable abundances

2. Particle acceleration at astrophysical shocks: A theory of cosmic ray origin

3. Temperature map computation for X-ray clusters of galaxies

4. Temperature structure of the intergalactic medium within seven nearby and bright clusters of galaxies observed with XMM-Newton

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1. Resolving high-z galaxy cluster properties through joint X-ray and millimeter analysis: Case study of SPT-CLJ0615-5746;Astronomy & Astrophysics;2024-08

2. The heart of galaxy clusters: Demographics and physical properties of cool-core and non-cool-core halos in the TNG-Cluster simulation;Astronomy & Astrophysics;2024-07

3. A Rare, Strong Shock Front in the Merging Cluster SPT-CLJ 2031-4037;The Astrophysical Journal;2024-07-01

4. A Deep uGMRT View of the Ultra-steep Spectrum Radio Halo in A521;The Astrophysical Journal;2024-02-01

5. Post-processing of galaxies due to major cluster mergers;Astronomy & Astrophysics;2023-12

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