Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12666/153
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dc.rights.licenseCopyright © 2020, Oxford University Press-
dc.contributor.authorScourfield, M.-
dc.contributor.authorViti, S.-
dc.contributor.authorGarcía Burillo, S.-
dc.contributor.authorSaintonge, A.-
dc.contributor.authorCombes, F.-
dc.contributor.authorFuente, A.-
dc.contributor.authorHenkel, C.-
dc.contributor.authorAlonso Herrero, A.-
dc.contributor.authorHarada, N.-
dc.contributor.authorTakano, S.-
dc.contributor.authorNakajima, T.-
dc.contributor.authorMartín, S.-
dc.contributor.authorKrips, M.-
dc.contributor.authorVan der Werf, P. P.-
dc.contributor.authorAalto, S.-
dc.contributor.authorUsero, A.-
dc.contributor.authorKohno, K.-
dc.contributor.otherUnidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737-
dc.date.accessioned2021-04-08T07:29:03Z-
dc.date.available2021-04-08T07:29:03Z-
dc.date.issued2020-07-02-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society 496: 5308- 5329 (2020)es
dc.identifier.issn1365-2966-
dc.identifier.otherhttps://academic.oup.com/mnras/article-abstract/496/4/5308/5866511-
dc.identifier.urihttp://hdl.handle.net/20.500.12666/153-
dc.descriptionThis paper makes use of the following ALMA data: ADS/JAO.ALMA#2011.0.00083.S, ADS/JAO.ALMA#2013.1.00055.S, ADS/JAO.ALMA#2015.1.01144.S. ALMA is a partnership of European Southern Observatory (ESO) (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), MOST and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. SGB, AA-H, and AU acknowledge support from grant - PGC2018094671-B-I00 (MCIU/AEI/FEDER, UE). AAH work was done under project No. MDM-2017-0737 Unidad de Excelencia "Maria de Maeztu"- Centro de Astrobiologia (INTA-CSIC).es
dc.description.abstractWe present results from Atacama Large Millimeter/submillimeter Array (ALMA) observations of CS from the nearby galaxy NGC 1068 (∼14 Mpc). This Seyfert 2 barred galaxy possesses a circumnuclear disc (CND, r ∼ 200 pc) and a starburst ring (SB ring, r ∼ 1.3 kpc). These high-resolution maps (∼0.5 arcsec, ∼35 pc) allow us to analyse specific sub-regions in the galaxy and investigate differences in line intensity ratios and physical conditions, particularly those between the CND and SB ring. Local thermodynamic equilibrium (LTE) analysis of the gas is used to calculate CS densities in each sub-region, followed by the non-LTE analysis conducted using the radiative transfer code RADEX to fit observations and constrain gas temperature, CS column density and hydrogen density. Finally, the chemical code UCLCHEM is used to reconstruct the gas, allowing an insight into its origin and chemical history. The density of hydrogen in the CND is found to be ≥105 cm−2, although exact values vary, reaching 106 cm−2 at the active galactic nucleus. The conditions in the two arms of the SB ring appear similar to one another, though the density found (∼104 cm−2) is lower than in the CND. The temperature in the CND increases from east to west, and is also overall greater than found in the SB ring. These modelling methods indicate the requirement for multiphase gas components in order to fit the observed emission over the galaxy. A larger number of high-resolution transitions across the SLED may allow for further constraining of the conditions, particularly in the SB ring.es
dc.description.sponsorshipThis paper makes use of the following ALMA data: ADS/JAO.ALMA#2011.0.00083.S, ADS/JAO.ALMA#2013.1.00055.S, ADS/JAO.ALMA#2015.1.01144.S. ALMA is a partnership of European Southern Observatory (ESO) (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), MOST and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. SGB, AA-H, and AU acknowledge support from grant - PGC2018094671-B-I00 (MCIU/AEI/FEDER, UE). AAH work was done under project No. MDM-2017-0737 Unidad de Excelencia "Maria de Maeztu"- Centro de Astrobiologia (INTA-CSIC).es
dc.language.isoenges
dc.publisherOxford Academics: Blackwell Publishinges
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-094671-B-I00/ES/EVOLUCION DE GALAXIAS Y SUS AGUJEROS NEGROS CON ALTA RESOLUCION ESPACIAL: FEEDBACK, EL TORO Y FORMACION ESTELAR/-
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internationales
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/-
dc.subjectGalaxies: individuales
dc.subjectNGC 1068es
dc.subjectGalaxies: nucleies
dc.subjectradio lineses
dc.subjectAlma observationses
dc.subjectChemistryes
dc.titleALMA observations of CS in NGC 1068: Chemistry and excitationes
dc.typeinfo:eu-repo/semantics/articlees
dc.contributor.orcidAlonso Herrero, A. [0000-0001-6794-2519]-
dc.identifier.doi10.1093/mnras/staa1891-
dc.identifier.e-issn0035-8711-
dc.contributor.funderAgencia Estatal de Investigación (AEI)-
dc.description.peerreviewedPeer reviewes
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
dc.type.coarhttp://purl.org/coar/resource_type/c_6501-
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