Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/30704
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Gallimore, Jack F. | en_US |
dc.contributor.author | Elitzur, Moshe | en_US |
dc.contributor.author | Maiolino, Roberto | en_US |
dc.contributor.author | Marconi, Alessandro | en_US |
dc.contributor.author | O'Dea, Christopher P. | en_US |
dc.contributor.author | Lutz, Dieter | en_US |
dc.contributor.author | Baum, Stefi A. | en_US |
dc.contributor.author | NIKUTTA, ROBERT | en_US |
dc.contributor.author | Impellizzeri, C. M. V. | en_US |
dc.contributor.author | Davies, Richard | en_US |
dc.contributor.author | Kimball, Amy E. | en_US |
dc.contributor.author | Sani, Eleonora | en_US |
dc.date.accessioned | 2021-03-15T12:26:51Z | - |
dc.date.available | 2021-03-15T12:26:51Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 2041-8205 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/30704 | - |
dc.description.abstract | We have detected in ALMA observations CO J=6\to 5 emission from the nucleus of the Seyfert galaxy NGC 1068. The low-velocity (up to ±70 km s<SUP>-1</SUP> relative to systemic) CO emission resolves into a 12 × 7 pc structure, roughly aligned with the nuclear radio source. Higher-velocity emission (up to ±400 km s<SUP>-1</SUP>) is consistent with a bipolar outflow in a direction nearly perpendicular (≃80°) to the nuclear disk. The position-velocity diagram shows that in addition to the outflow, the velocity field may also contain rotation about the disk axis. These observations provide compelling evidence in support of the disk-wind scenario for the active galactic nucleus obscuring torus. | en_US |
dc.language.iso | eng | en_US |
dc.title | High-velocity Bipolar Molecular Emission from an AGN Torus | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/2041-8205/829/1/L7 | en_US |
dc.identifier.scopus | 2-s2.0-84989193772 | en_US |
dc.identifier.isi | 000385412000007 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/2041-8205/829/1/L7 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 829 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | L7 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE ASTROPHYSICAL JOURNAL LETTERS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2016ApJ...829L...7G | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_8 Formation and evolution of galaxies | 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. Arcetri | - |
crisitem.author.orcid | 0000-0002-9889-4238 | - |
crisitem.journal.journalissn | 2041-8205 | - |
crisitem.journal.ance | E196528 | - |
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Gallimore_2016_ApJL_829_L7.pdf | PDF editoriale | 2.89 MB | Adobe PDF | Visualizza/apri |
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