Reconciling AGN-star formation, the Soltan argument, and Meier's paradox

We provide a theoretical context for understanding the recent work of Kalfountzou et al (2014) showing that star formation is enhanced at lower optical luminosity in radio loud quasars. Our proposal for coupling the assumption of collimated FRII quasar jet-induced star formation with lower accretion...

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Bibliographic Details
Published inarXiv.org
Main Authors Garofalo, David, Kim, Matthew I, Christian, Damian J, Hollingworth, Emily, Lowery, Aaron, Harmon, Matthew
Format Paper Journal Article
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 17.12.2015
Subjects
Active galactic nuclei
Active galaxies
Collimation
Deposition
Luminosity
Physics - Astrophysics of Galaxies
Physics - High Energy Astrophysical Phenomena
Quasars
Red shift
Star & galaxy formation
Star formation
Stellar evolution
Supermassive black holes
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Summary:We provide a theoretical context for understanding the recent work of Kalfountzou et al (2014) showing that star formation is enhanced at lower optical luminosity in radio loud quasars. Our proposal for coupling the assumption of collimated FRII quasar jet-induced star formation with lower accretion optical luminosity, also explains the observed jet power peak in active galaxies at higher redshift compared to the peak in accretion power, doing so in a way that predicts the existence of a family of radio quiet AGN associated with rapidly spinning supermassive black holes at low redshift, as mounting observations suggest. The relevance of this work lies in its promise to explain the observed cosmological evolution of accretion power, jet power, and star formation, in a way that is both compatible with the Soltan argument and resolves the so-called `Meier Paradox'.
ISSN:2331-8422
DOI:10.48550/arxiv.1512.05452