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dc.contributor.authorCernicharo, José-
dc.contributor.authorCabezas, Carlos-
dc.contributor.authorPardo Carrión, Juan Ramón-
dc.contributor.authorAgúndez, Marcelino-
dc.contributor.authorBermúdez, Celina-
dc.contributor.authorVelilla Prieto, L.-
dc.contributor.authorTercero, F.-
dc.contributor.authorLópez-Pérez, J. A.-
dc.contributor.authorGallego, J. D.-
dc.contributor.authorFonfría, José Pablo-
dc.contributor.authorQuintana-Lacaci, G.-
dc.contributor.authorGuélin, M.-
dc.contributor.authorEndo, Y.-
dc.date.accessioned2020-03-05T11:46:54Z-
dc.date.available2020-03-05T11:46:54Z-
dc.date.issued2019-09-23-
dc.identifierdoi: 10.1051/0004-6361/201936372-
dc.identifierissn: 1432-0746-
dc.identifier.citationAstronomy and Astrophysics 630: L2 (2019)-
dc.identifier.urihttp://hdl.handle.net/10261/202868-
dc.description10 pags., 5 figs., 7 tabs., 5 apps.-
dc.description.abstractWe report on the detection of two series of harmonically related doublets in IRC+10216. From the observed frequencies, the rotational constant of the first series is B = 1380.888 MHz and that of the second series is B = 1381.512 MHz. The two series correspond to two species with a 2Σ electronic ground state. After considering all possible candidates, and based on quantum chemical calculations, the first series is assigned to MgC3N and the second to MgC4H. For the latter species, optical spectroscopy measurements support its identification. Unlike diatomic metal-containing molecules, the line profiles of the two new molecules indicate that they are formed in the outer layers of the envelope, as occurs for MgNC and other polyatomic metal-cyanides. We also confirm the detection of MgCCH that was previously reported from the observation of two doublets. The relative abundance of MgC3N with respect to MgNC is close to one while that of MgC4H relative to MgCCH is about ten. The synthesis of these magnesium cyanides and acetylides in IRC+10216 can be explained in terms of a two-step process initiated by the radiative association of Mg+ with large cyanopolyynes and polyynes followed by the dissociative recombination of the ionic complexes.-
dc.description.sponsorshipThe Spanish authors thank the Ministerio de Ciencia Innovación y Universidades for funding support from the CONSOLIDER-Ingenio program “ASTROMOL” CSD 2009-00038, AYA2012-32032, AYA2016-75066-C2-1-P. We also thank ERC for funding through grant ERC-2013-Syg610256-NANOCOSMOS. MA thanks the Ministerio de Ciencia Innovación y Universidades for the Ramón y Cajal grant RyC-2014-16277. CB thanks the Ministerio de Ciencia Innovación y Universidades for the Juan de la Cierva grant FJCI-2016-27983. LVP acknowledges support from the Swedish Research Council and from ERC consolidator grant 614-
dc.languageeng-
dc.publisherSpringer Nature-
dc.relationinfo:eu-repo/grantAgreement/EC/FP7/610256-
dc.relationinfo:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/FJCI-2016-27983-
dc.relationinfo:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-75066-C2-1-P-
dc.relation.isversionofPublisher's version-
dc.rightsopenAccess-
dc.subjectMolecular data-
dc.subjectLine: identification-
dc.subjectStars: carbon-
dc.subjectCircumstellar matter-
dc.subjectStars: individual: IRC+10216-
dc.subjectAstrochemistry-
dc.titleDiscovery of two new magnesium-bearing species in IRC+10216: MgC3N and MgC4H-
dc.typeartículo-
dc.identifier.doi10.1051/0004-6361/201936372-
dc.relation.publisherversionhttp://dx.doi.org/10.1051/0004-6361/201936372-
dc.date.updated2020-03-05T11:46:54Z-
dc.contributor.funderMinisterio de Ciencia e Innovación (España)-
dc.contributor.funderEuropean Commission-
dc.contributor.funderMinisterio de Ciencia, Innovación y Universidades (España)-
dc.contributor.funderSwedish Research Council-
dc.contributor.funderMinisterio de Economía y Competitividad (España)-
dc.relation.csic-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000780es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003329es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100004837es_ES
dc.identifier.pmid31579315-
dc.type.coarhttp://purl.org/coar/resource_type/c_6501es_ES
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextopen-
item.openairetypeartículo-
item.fulltextWith Fulltext-
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