Cluster Outskirts and Their Connection to the Cosmic Web
Handbook of X-ray and Gamma-ray Astrophysics, Page: 4813-4849
2024
- 17Captures
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Metrics Details
- Captures17
- Readers17
- 17
Book Chapter Description
We review the latest developments in our X-ray observational and theoretical understanding of the outskirts of galaxy cluster, and their connection to the cosmic web. The faint cluster outskirts are challenging regions to observe in Xrays, requiring highly sensitive telescopes with low and stable background levels. We present our latest understanding of the thermodynamic profiles of clusters in the outskirts and the biases that gas clumping and non-thermal pressure support can introduce. Features in the outskirts due to merging activity are discussed, along with the chemical enrichment of the outskirts ICM. We describe future prospects for X-ray observations to explore further out in the cluster outskirts and probe their connections to the cosmic web.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=85207555164&origin=inward; http://dx.doi.org/10.1007/978-981-19-6960-7_120; https://link.springer.com/10.1007/978-981-19-6960-7_120; https://dx.doi.org/10.1007/978-981-19-6960-7_120; https://link.springer.com/referenceworkentry/10.1007/978-981-19-6960-7_120
Springer Science and Business Media LLC
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