Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/31503
DC Field | Value | Language |
---|---|---|
dc.contributor.author | MAGLIOCCHETTI, MANUELA | en_US |
dc.contributor.author | Paola Popesso | en_US |
dc.contributor.author | Marcella Brusa | en_US |
dc.contributor.author | Mara Salvato | en_US |
dc.date.accessioned | 2022-02-28T15:37:14Z | - |
dc.date.available | 2022-02-28T15:37:14Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31503 | - |
dc.description.abstract | Investigations of the population of radio-active AGN up to z=3.5 not only show that these sources are hosted by galaxies of very large, M*>1010.5 Msun, stellar masses, but also that at all redshifts they reside in very massive dark matter halos, comparable to those associated with groups-to-clusters of galaxies. This result is found both via clustering studies and by directly pinpointing such sources to the cosmological structures they belong to. We also show how intense star-forming activity is encountered in the overwhelming majority of z>1 (massive) galaxies hosts of radio-active AGN, and how this activity is only halted by nuclear feedbacks in the relatively local universe. What emerges from our work is a scenario whereby physical processes at sub-pc/pc (e.g. AGN emission) and kpc scales strongly influence the large-scale structure behavior of the AGN and its host. | en_US |
dc.format | 1 - Video | en_US |
dc.format.medium | 1 - Digitale | en_US |
dc.language.iso | eng | en_US |
dc.title | Hosts and environments of radio-active AGN | en_US |
dc.type | Multimedia | - |
dc.identifier.doi | 10.5281/zenodo.1472829 | en_US |
dc.identifier.url | https://zenodo.org/record/1472829#.X23ujx1S-og | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.numberofpages | 13 | en_US |
dc.type.referee | REF_0 | en_US |
dc.description.numberofauthors | 4 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.type.invited | no | en_US |
dc.relation.conferencename | AGN13: Beauty and the Beast. The 13th Italian meeting on Active Galactic Nuclei | en_US |
dc.relation.conferenceplace | Milano (IT) | en_US |
dc.relation.conferencedate | 9-12 October, 2018 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 298 Altro | - |
dc.identifier.adsbibcode | 2018agn..confE..26M | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Multimedia | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.orcid | 0000-0001-9158-4838 | - |
Appears in Collections: | 4.09 Prodotti multimediali |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Magliocchetti-AGN13_talk.pdf | Talk | 18.65 MB | Adobe PDF | View/Open |
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Items in DSpace are published in Open Access, unless otherwise indicated.