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dc.rights.licensepublished by MDPI-
dc.contributor.authorSánchez Contreras, C.-
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.accessioned2021-04-12T08:54:55Z-
dc.date.available2021-04-12T08:54:55Z-
dc.date.issued2020-03-10-
dc.identifier.citationGalaxies 8(1): 21(2020)es
dc.identifier.otherhttps://www.mdpi.com/2075-4434/8/1/21-
dc.identifier.urihttp://hdl.handle.net/20.500.12666/229-
dc.description.abstractThis is a non-comprehensive review of observations of pre-Planetary Nebulae (pPNe) and young Planetary Nebulae (yPNe) at (sub)mm-wavelengths, a valuable window for probing multi-phased gas and dust in these objects. This contribution focuses on observations of molecular lines (from carbon monoxide—CO—and other species), and briefly at the end, on hydrogen radio recombination lines from the emerging H ii regions at the center of yPNe. The main goal of this contribution is to show the potential of (sub)mm-wavelength observations of pPNe/yPNe to help the community to devise and develop new observational projects that will bring us closer to a better understanding of these latest stages of the evolution of low-to-intermediate (∼0.8–8es
dc.description.sponsorshipThis work has been partially supported by the Spanish MINECO through grants AYA2016-75066-C2-1-P and AYA2016-78994-P and by the European Research Council through ERC grant 610256: NANOCOSMOS; With funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737).es
dc.language.isoenges
dc.publisherMultidisciplinary Digital Publishing Institute (MDPI)es
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-75066-C2-1-P/ES/EVOLUCION FISICA Y QUIMICA DEL MEDIO INTERESTELAR, CIRCUNESTELAR, Y PLANETARIO/-
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-78994-P/ES/EL SURGIMIENTO DE LA SIMETRIA AXIAL EN NEBULOSAS DE ESTRELLAS EVOLUCIONADAS/-
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International*
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.subjectAGB and post AGB starses
dc.subjectCircumstellar matteres
dc.subjectWinds and outflowses
dc.subjectMass-losses
dc.subjectJetses
dc.title(Sub)mm-Wavelength Observations of Pre-Planetary Nebulae and Young Planetary Nebulaees
dc.typeinfo:eu-repo/semantics/articlees
dc.contributor.orcid0000-0002-6341-592X-
dc.identifier.doi10.3390/galaxies8010021-
dc.identifier.e-issn2075-4434-
dc.contributor.funderNational Aeronautics and Space Administration (NASA)-
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-
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/FP7/610256-
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