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Morphologies of z ∼ 0.7 AGN host galaxies in CANDELS: no trend of merger incidence with AGN luminosity [PDF]
Monthly Notices of the Royal Astronomical Society, 2014 PS would like to acknowledge funding through grant ASI I/005/11/0. DKoo would like to acknowledge funding through grant NSF AST-0808133. SJ acknowledges financial support from the EC through an ERC grant StG-257720.The processes that trigger active ...
Jeyhan S. Kartaltepe +2 more
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New Astronomy Reviews, 2008 A series of four lectures presented at the 2007 summer school on "Active Galactic Nuclei at the highest angular resolution: theory and observations" held in Torun, Poland.
Sylvain Veilleux
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THE HOST GALAXIES OF 23,000 AGN
Multiwavelength AGN Surveys, 2004We examine the relationship between galaxies, supermassive black holes and AGN using a sample of ~ 2 3 , 0 0 0 narrow-emission-line (Type 2) AGN drawn from a sample of ~ 1 2 3 , 0 0 0 galaxies from the Sloan Digital Sky Survey. We have studied how AGN host properties compare to those of normal galaxies and how they depend on the luminosity of the ...
Heckman, T., Kauffmann, G.
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The mass–metallicity and fundamental metallicity relations in non-AGN and AGN-host galaxies [PDF]
Monthly Notices of the Royal Astronomical SocietyGalaxies' stellar masses, gas-phase oxygen abundances (metallicity), and star formation rates (SFRs) obey a series of empirical correlations, most notably the mass-metallicity relation (MZR) and fundamental metallicity relation (FZR), which relates ...
Zefeng Li, Lisa Kewley, Kathryn Grasha
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The coevolution of the AGNs and their host galaxies
2021Η παρούσα διδακτορική διατριβή, πραγματεύεται τη μελέτη της σχέσης του Eνεργού Γαλαξιακού Πυρήνα (AGN) με τον περιβάλλοντα γαλαξία. Μελέτες των τελευταίων δεκαετιών έχουν οδηγήσει στο συμπέρασμα ότι υπάρχει άρρηκτη σχέση ανάμεσα στους γαλαξίες και στις υπερμεγέθεις μελανές οπές (SMBHs) που φιλοξενούν στο κέντρο τους.
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AGN, host galaxies, and starbursts
Proceedings of the International Astronomical Union, 2019AbstractAGN by definition live in galaxies. Despite a long history of studies, there is still much ongoing research into the interplay of the nucleus and the host galaxy, how do they affect each other, how is their evolution intertwined. This review will briefly go over the historical developments behind the current understanding of AGN host galaxies ...
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Two-Dimensional Modeling of AGN Host Galaxies
2001We present a method to model the two-dimensional light distribution of Quasar and Seyfert 1 host galaxies by multi-component fitting. The method has been tested on a large set of simulations, showing its ability to recover total fluxes and morphological properties within the observational errors.
Kuhlbrodt, B. +2 more
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AGN and the Characteristics of their Host Galaxies
2013The vast majority of optically identified active galactic nuclei (AGNs) in the local universe reside in host galaxies with prominent bulges, supporting the hypothesis that black hole formation and growth is fundamentally connected to the buildup of galaxy bulges.
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Host Galaxies of Radio-Loud AGN
1997We are studying the host galaxies and cluster environments of a sample of radio-loud AGN. The sample is large enough to compare sub-samples (quasars, FRI and FRII radio galaxies, RBL and XBL). First results show that elliptical host galaxies fall on the μ e — r e relation of bright elliptical galaxies.
Josef W. Fried, Jochen Heidt
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Galaxies Hosting AGN Activity and Their Environments
2010Nuclear activity in galaxies (AGN) has recently started attracting a broader attention, in one hand, because of the relationship found between the mass of the central spheroidal regions of galaxies and the black holes they host. On the other hand, the output energy provided by AGN (feedback) seems to be crucial for current cosmological simulations to ...
Isabel Márquez, Josefa Masegosa
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