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The relation between the diffuse X-ray luminosity and the radio power of the central AGN in galaxy groups

dc.contributor.authorJarvis, M.
dc.contributor.authorPasini, T.
dc.contributor.authorBruggen, M.
dc.date.accessioned2021-02-08T09:30:38Z
dc.date.available2021-02-08T09:30:38Z
dc.date.issued2020
dc.identifier.citationJarvis, M. et al. (2020). The relation between the diffuse X-ray luminosity and the radio power of the central AGN in galaxy groups. Monthly Notices of the Royal Astronomical Society, 497( 2), 2163–2174en_US
dc.identifier.issn1365-2966
dc.identifier.urihttps://doi.org/10.1093/mnras/staa2049
dc.identifier.urihttp://hdl.handle.net/10566/5852
dc.description.abstractOur understanding of how active galactic nucleus feedback operates in galaxy clusters has improved in recent years owing to large efforts in multiwavelength observations and hydrodynamical simulations. However, it is much less clear how feedback operates in galaxy groups, which have shallower gravitational potentials. In this work, using very deep Very Large Array and new MeerKAT observations from the MIGHTEE survey, we compiled a sample of 247 X-ray selected galaxy groups detected in the COSMOS field. We have studied the relation between the X-ray emission of the intra-group medium and the 1.4 GHz radio emission of the central radio galaxy.en_US
dc.language.isoenen_US
dc.publisherOxford University Pressen_US
dc.subjectGalaxies: clusters: generalen_US
dc.subjectGalaxies: clusters: intracluster mediumen_US
dc.subjectGalaxies: groups: generalen_US
dc.subjectRadio continuum: galaxiesen_US
dc.subjectX-rays: galaxies: clustersen_US
dc.titleThe relation between the diffuse X-ray luminosity and the radio power of the central AGN in galaxy groupsen_US
dc.typeArticleen_US


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