Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power
Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power
About this item
Full title
Author / Creator
Kalfountzou, E , Stevens, J A , Jarvis, M J , Hardcastle, M J , Wilner, D , Elvis, M , Page, M J , Trichas, M and Smith, D J B
Publisher
Ithaca: Cornell University Library, arXiv.org
Journal title
Language
English
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Publication information
Publisher
Ithaca: Cornell University Library, arXiv.org
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Scope and Contents
Contents
Several studies support the existence of a link between the AGN and star formation activity. Radio jets have been argued to be an ideal mechanism for direct interaction between the AGN and the host galaxy. A drawback of previous surveys of AGN is that they are fundamentally limited by the degeneracy between redshift and luminosity in flux-density l...
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Full title
Observational evidence that positive and negative AGN feedback depends on galaxy mass and jet power
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Record Identifier
TN_cdi_proquest_journals_2075709155
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2075709155
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.1706.02334
