Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/31226
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Wagg, J. | en_US |
dc.contributor.author | Aravena, M. | en_US |
dc.contributor.author | Brisbin, D. | en_US |
dc.contributor.author | Valtchanov, I. | en_US |
dc.contributor.author | Carilli, C. | en_US |
dc.contributor.author | Daddi, E. | en_US |
dc.contributor.author | Dannerbauer, H. | en_US |
dc.contributor.author | DECARLI, ROBERTO | en_US |
dc.contributor.author | Díaz-Santos, T. | en_US |
dc.contributor.author | Riechers, D. | en_US |
dc.contributor.author | Sargent, M. | en_US |
dc.contributor.author | Walter, F. | en_US |
dc.date.accessioned | 2021-12-10T14:58:41Z | - |
dc.date.available | 2021-12-10T14:58:41Z | - |
dc.date.issued | 2020 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31226 | - |
dc.description.abstract | We present Herschel-PACS spectroscopy of four main-sequence star-forming galaxies at z ∼ 1.5. We detect [OI]63-=μm line emission in BzK-21000 at z = 1.5213, and measure a line luminosity, $L_{\rm [O\, {\small I}]63\, \mu m} = (3.9\pm 0.7)\times 10^9$ -=L<SUB>⊙</SUB>. Our PDR modelling of the interstellar medium in BzK-21000 suggests a UV radiation field strength, G ∼ 320G<SUB>0</SUB>, and gas density, n ∼ 1800-=cm<SUP>-3</SUP>, consistent with previous LVG modelling of the molecular CO line excitation. The other three targets in our sample are individually undetected in these data, and we perform a spectral stacking analysis which yields a detection of their average emission and an [O-=I]63-=μm line luminosity, $L_{\rm [O\, {\small I}]63\, \mu m} = (1.1\pm 0.2)\times 10^9$ -=L<SUB>⊙</SUB>. We find that the implied luminosity ratio, $L_{\rm [O\, {\small I}]63\, \mu m}/L_{\rm IR}$ , of the undetected BzK-selected star-forming galaxies broadly agrees with that of low-redshift star-forming galaxies, while BzK-21000 has a similar ratio to that of a dusty star-forming galaxy at z ∼ 6. The high [O-=I]63-=μm line luminosities observed in BzK-21000 and the z ∼ 1-3 dusty and sub-mm luminous star-forming galaxies may be associated with extended reservoirs of low density, cool neutral gas. | en_US |
dc.language.iso | eng | en_US |
dc.title | Observations of [OI]63-=μm line emission in main-sequence galaxies at z ∼ 1.5 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/staa2884 | en_US |
dc.identifier.scopus | 2-s2.0-85096899279 | en_US |
dc.identifier.isi | WOS:000587762900017 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/499/2/1788/5909056 | en_US |
dc.identifier.url | http://arxiv.org/abs/2009.08984v1 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 499 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 1788 | en_US |
dc.relation.lastpage | 1794 | 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 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2020MNRAS.499.1788W | 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 | 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.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0002-2662-8803 | - |
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