Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/30704
DC Field | Value | Language |
---|---|---|
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 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Gallimore_2016_ApJL_829_L7.pdf | PDF editoriale | 2.89 MB | Adobe PDF | View/Open |
Page view(s)
51
checked on Apr 18, 2024
Download(s)
13
checked on Apr 18, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.