High Energy Emission from Clusters, Groups, and Filaments: Current Observations and Future Prospects

A special issue of Universe (ISSN 2218-1997). This special issue belongs to the section "Galaxies and Clusters".

Deadline for manuscript submissions: closed (31 December 2023) | Viewed by 2226

Special Issue Editor


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Guest Editor
Physics Department, University of Maryland, Baltimore County, Baltimore, MD 21250, USA
Interests: high energy emission from clusters, groups, and filaments; galaxy evolution; astrobiology

Special Issue Information

Dear Colleagues,

From the HEAO satellites nearly 50 years ago to the present cadre of active observatories— Chandra, XMM, Suzaku, NuStar, and eRosita—our view of the physics of structure formation has changed enormously. X-ray observations of superclusters, clusters, groups, and filaments have provided unprecedented insight into structure formation. Given the huge increase in spectral and spatial resolution, as well as sensitivity that has been achieved during this time, it is especially timely to present new results with an eye toward the most important issues in structure formation that should be addressed by future missions and the telescope–detector requirements needed to carry them out. In this Special Issue, we solicit contributions that address high energy emission from clusters, groups, and filaments: current observations and future prospects.

Topics include (but are not limited to):

  • The physics of mergers and accretions including thermodynamic quantities (T,P,S) based on X-ray observations;
  • Shock physics in the intracluster medium;
  • The central region of clusters, in particular the AGN-ICM connection seen in X-ray cavities;
  • Searches for the non-thermal signature in structure formation;
  • Studies of the outskirts of the intracluster medium, including non-hydrostatic gas, accretion shocks, cool baryons;
  • Studies related to uniformity of the average abundance in clusters and spatial deviations from solar abundance;
  • Filamentary baryons;
  • Structure in supercluster/filament systems;
  • High redshift clusters of galaxies;
  • The requirements for future X-ray missions (e.g., AXIS, Athena) to address the most compelling issues for galaxy clusters.

Prof. Dr. Mark Henriksen
Guest Editor

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Keywords

  • clusters of galaxies
  • X-ray emission
  • superclusters
  • filaments
  • non-thermal emission
  • structure formation
  • future missions
  • intracluster medium
  • X-ray cavities
  • cluster atmosphere

Published Papers (2 papers)

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Research

14 pages, 709 KiB  
Article
Tracking Dusty Cloud Crushed by a Hot Flow
by Svyatoslav Dedikov and Evgenii Vasiliev
Universe 2024, 10(4), 155; https://doi.org/10.3390/universe10040155 - 26 Mar 2024
Viewed by 510
Abstract
The destructionof clouds by strong shocks and hot winds is the key process responsible for the transporting of metals and dust from the ISM to the ICM/IGM, and establishing the multiphase structure in and around galaxies. In this work, we perform a detailed [...] Read more.
The destructionof clouds by strong shocks and hot winds is the key process responsible for the transporting of metals and dust from the ISM to the ICM/IGM, and establishing the multiphase structure in and around galaxies. In this work, we perform a detailed analysis of this process using two different approaches for tracking the cloud material (gas and dust): the so-called ‘colored’ fluid, and the Lagrangian (trace) particles. We find that for the clouds in the hot phase (T>105 K), the two methods produce significantly different mass fractions and velocities of the cloud material. In contrast, the two methods produce similar results for the clouds that are in the warm/cold phases (T<105 K). We find that the Kelvin–Helmholtz instability is suppressed in the warm clouds of size ∼100 pc and metallicity Z> 0.1Zduetoeffectivegascooling.ThiscausesadelayinthedestructionofsuchcloudsthatareinteractingwiththehotICMflow.WedemonstratethatthedustparticlesthatareevacuatedfromtheirparentcloudstothehotmediumshowdifferentdynamicswhencomparedtothatoftheLagrangian(trace)particles.Ourresultsindicatethatthedustgrainssweptouttothehotgasaredestroyed. Full article
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20 pages, 1010 KiB  
Article
VLBI Analysis of a Potential High-Energy Neutrino Emitter Blazar
by Janka Kőmíves, Krisztina Éva Gabányi, Sándor Frey and Emma Kun
Universe 2024, 10(2), 78; https://doi.org/10.3390/universe10020078 - 06 Feb 2024
Viewed by 1080
Abstract
Recent studies suggest that high-energy neutrinos can be produced in the jets of blazars, radio-loud active galactic nuclei (AGN) with jets pointing close to the line of sight. Due to the relatively poor angular resolution of current neutrino detectors, several sources can be [...] Read more.
Recent studies suggest that high-energy neutrinos can be produced in the jets of blazars, radio-loud active galactic nuclei (AGN) with jets pointing close to the line of sight. Due to the relatively poor angular resolution of current neutrino detectors, several sources can be regarded as the possible counterpart of a given neutrino event. Therefore, follow-up observations of counterpart candidates in the electromagnetic regime are essential. Since the Very Long Baseline Interferometry (VLBI) technique provides the highest angular resolution to study the radio jets of blazars, a growing number of investigations are being conducted to connect individual blazars to given high-energy neutrino events. We analyzed more than 20 years of available archival VLBI data of the blazar CTD 74, which has been listed as a possible counterpart of a neutrino event. Using cm-wavelength data, we investigated the jet structure, determined the apparent speed of jet components, and the core flux density before and after the neutrino event. Our results indicate stationary jet features and a significant brightening of the core after the neutrino event. Full article
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