Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26067
DC Field | Value | Language |
---|---|---|
dc.contributor.author | MARZIANI, Paola | en_US |
dc.contributor.author | Sulentic, J. W. | en_US |
dc.contributor.author | STIRPE, Giovanna Maria | en_US |
dc.contributor.author | Dultzin, D. | en_US |
dc.contributor.author | Del Olmo, A. | en_US |
dc.contributor.author | Martínez-Carballo, M. A. | en_US |
dc.date.accessioned | 2020-06-15T16:05:41Z | - |
dc.date.available | 2020-06-15T16:05:41Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 0004-640X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26067 | - |
dc.description.abstract | [OIII]λ 5007 "blue outliers"—that are suggestive of outflows in the narrow line region of quasars—appear to be much more common at intermediate z (high luminosity) than at low z. About 40~% of quasars in a Hamburg ESO intermediate z sample of 52 sources qualify as "blue outliers" (i.e., quasars with [OIII]λλ 4959,5007 lines showing large systematic blueshifts with respect to rest frame). We discuss major findings on what has become an intriguing field in active galactic nuclei research and stress the relevance of "blue outliers" to feedback and host galaxy evolution. | en_US |
dc.language.iso | eng | en_US |
dc.title | Blue outliers among intermediate redshift quasars | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1007/s10509-015-2590-2 | en_US |
dc.identifier.scopus | 2-s2.0-84948748449 | en_US |
dc.identifier.isi | 000367516500003 | en_US |
dc.identifier.url | https://link.springer.com/article/10.1007%2Fs10509-015-2590-2 | en_US |
dc.identifier.url | https://arxiv.org/abs/1511.07138 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 361 | en_US |
dc.relation.firstpage | 3 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | ESP | en_US |
dc.contributor.country | MEX | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | ASTROPHYSICS AND SPACE SCIENCE | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2016Ap&SS.361....3M | 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 | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0002-6058-4912 | - |
crisitem.author.orcid | 0000-0002-3702-8731 | - |
crisitem.journal.journalissn | 0004-640X | - |
crisitem.journal.ance | E016259 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
1511.07138.pdf | postprint | 1.75 MB | Adobe PDF | View/Open |
Marziani2015_Article_BlueOutliersAmongIntermediateR.pdf | [Administrators only] | 1.89 MB | Adobe PDF |
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