Black hole and galaxy co-evolution in radio-loud AGN at z ~ 0.3-4
Black hole and galaxy co-evolution in radio-loud AGN at z ~ 0.3-4
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Contents
There exists a well known relation between the mass of the supermassive black hole (SMBH) in the center of galaxies and their bulge mass or central velocity dispersion. This suggests a co-evolution between SMBH and their galaxy hosts. Our aim is to study this relation specifically for radio loud galaxies, and as a function of redshift \(z\). We sel...
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Full title
Black hole and galaxy co-evolution in radio-loud AGN at z ~ 0.3-4
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TN_cdi_proquest_journals_2765223633
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2765223633
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2301.05186
