Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/28028
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Antón, S. | en_US |
dc.contributor.author | CACCIANIGA, Alessandro | en_US |
dc.contributor.author | Bizzocchi, L. | en_US |
dc.contributor.author | Afonso, J. | en_US |
dc.date.accessioned | 2020-10-27T15:33:54Z | - |
dc.date.available | 2020-10-27T15:33:54Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 1824-8039 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/28028 | - |
dc.description.abstract | A fraction of Narrow Line Seyfert 1 galaxies (NLS1) are hosted by galaxies that present a disturbed morphology, in some cases hinting for merger processes, that are putative sources of gas replenishment. We have been investigating the poorly studied population of radio loud NLS1 (RL-NLS1) showing a flat radio spectrum, assumed to be the manifestation of the presence of a radio jet. In some of the objects the infrared emission is well fitted by a combination of an AGN component and an "active" host galaxy component like M82, the estimate SFR being in the LIRG/ULIRG range (10-500 Msun/year). In order to better characterize that component, we have been investigating the sub-millimeter/millimeter emission of the sources using APEX. Here we present the results concerning a pilot sample of 2 representative objects. | en_US |
dc.language.iso | eng | en_US |
dc.title | What is in a radio loud NLS1? | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.22323/1.328.0058 | en_US |
dc.identifier.scopus | 2-s2.0-85073732903 | en_US |
dc.identifier.url | https://pos.sissa.it/328/058/ | en_US |
dc.identifier.url | https://pos.sissa.it/328/ | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.firstpage | 58 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 4 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | PRT | en_US |
dc.relation.ispartofbook | Revisiting Narrow-Line Seyfert 1 Galaxies and their Place in the Universe | en_US |
dc.type.invited | no | en_US |
dc.relation.conferencename | Revisiting Narrow-Line Seyfert 1 Galaxies and their Place in the Universe | en_US |
dc.relation.conferenceplace | Padova | en_US |
dc.relation.conferencedate | 9-13 April, 2018 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | POS PROCEEDINGS OF SCIENCE | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.identifier.adsbibcode | 2018rnls.confE..58A | 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 | Conference paper | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.orcid | 0000-0002-2339-8264 | - |
crisitem.journal.journalissn | 1824-8039 | - |
crisitem.journal.ance | E188909 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
NLS1-2018_058.pdf | Pdf editoriale | 343.21 kB | Adobe PDF | View/Open |
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Items in DSpace are published in Open Access, unless otherwise indicated.