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    Reference Work Entry In depth

    AGN Feedback in Groups and Clusters of Galaxies

    Active galactic nuclei (AGN) feedback stands for the dramatic impact that a supermassive black hole can make on its environment. It has become an essential element of models that describe the formation and evo...

    Julie Hlavacek-Larrondo, Yuan Li in Handbook of X-ray and Gamma-ray Astrophysi… (2024)

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    Living Reference Work Entry In depth

    AGN Feedback in Groups and Clusters of Galaxies

    Active galactic nuclei (AGN) feedback stands for the dramatic impact that a supermassive black hole can make on its environment. It has become an essential element of models that describe the formation and evo...

    Julie Hlavacek-Larrondo, Yuan Li in Handbook of X-ray and Gamma-ray Astrophysi…

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    Article

    Constraining Gas Motions in the Intra-Cluster Medium

    The detailed velocity structure of the diffuse X-ray emitting intra-cluster medium (ICM) remains one of the last missing key ingredients in understanding the microphysical properties of these hot baryons and c...

    Aurora Simionescu, John ZuHone, Irina Zhuravleva, Eugene Churazov in Space Science Reviews (2019)

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    Article

    Astrophysics with the Spatially and Spectrally Resolved Sunyaev-Zeldovich Effects

    In recent years, observations of the Sunyaev-Zeldovich (SZ) effect have had significant cosmological implications and have begun to serve as a powerful and independent probe of the warm and hot gas that pervad...

    Tony Mroczkowski, Daisuke Nagai, Kaustuv Basu, Jens Chluba in Space Science Reviews (2019)

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    Article

    X-Ray Spectroscopy of Galaxy Clusters: Beyond the CIE Modeling

    X-ray spectra of galaxy clusters are dominated by the thermal emission from the hot intracluster medium. In some cases, besides the thermal component, spectral models require additional components associated, ...

    Liyi Gu, Irina Zhuravleva, Eugene Churazov, Frits Paerels in Space Science Reviews (2018)

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    Article

    Resonant Scattering of X-ray Emission Lines in the Hot Intergalactic Medium

    While very often a hot intergalactic medium (IGM) is optically thin to continuum radiation, the optical depth in resonant lines can be of order unity or larger. Resonant scattering in the brightest X-ray emiss...

    Eugene Churazov, Irina Zhuravleva, Sergey Sazonov, Rashid Sunyaev in Space Science Reviews (2010)

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    Chapter and Conference Paper

    The Cluster Abell 85 and its X-ray Filament Revisited by Chandra and XMM-Newton

    We have observed with XMM-Newton the extended 4 Mpc filament detected by the ROSAT PSPC south east of the cluster of galaxies Abell 85. We confirm the presence of an extended feature and find that the X-ray em...

    Florence Durret, Gastão B. Lima Neto in Soft X-Ray Emission from Clusters of Galax… (2004)