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(Sub)mm-Wavelength Observations of Pre-Planetary Nebulae and Young Planetary Nebulae

dc.contributor.authorSánchez Contreras, C.
dc.contributor.funderNational Aeronautics and Space Administration (NASA)
dc.contributor.funderAgencia Estatal de Investigación (AEI)
dc.contributor.orcid0000-0002-6341-592X
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.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.peerreviewedPeer reviewes
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.identifier.citationGalaxies 8(1): 21(2020)es
dc.identifier.doi10.3390/galaxies8010021
dc.identifier.e-issn2075-4434
dc.identifier.otherhttps://www.mdpi.com/2075-4434/8/1/21
dc.identifier.urihttp://hdl.handle.net/20.500.12666/229
dc.language.isoenges
dc.publisherMultidisciplinary Digital Publishing Institute (MDPI)es
dc.relationEVOLUCION FISICA Y QUIMICA DEL MEDIO INTERESTELAR, CIRCUNESTELAR, Y PLANETARIO
dc.relationEL SURGIMIENTO DE LA SIMETRIA AXIAL EN NEBULOSAS DE ESTRELLAS EVOLUCIONADAS
dc.relationNANOCOSMOS 610256
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.relation.projectIDinfo:eu-repo/grantAgreement/EC/FP7/610256
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International*
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.rights.licensepublished by MDPI
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.type.coarhttp://purl.org/coar/resource_type/c_6501
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion
dspace.entity.typePublication
oaire.awardNumberAYA2016-75066-C2-1-P
oaire.awardNumberAYA2016-78994-P
oaire.awardNumber610256
oaire.awardTitleEVOLUCION FISICA Y QUIMICA DEL MEDIO INTERESTELAR, CIRCUNESTELAR, Y PLANETARIO
oaire.awardTitleEL SURGIMIENTO DE LA SIMETRIA AXIAL EN NEBULOSAS DE ESTRELLAS EVOLUCIONADAS
oaire.awardTitleNANOCOSMOS 610256
oaire.awardURIhttps://digitalpro.inta.es/handle/123456789/1325
oaire.awardURIhttps://digitalpro.inta.es/handle/123456789/1431
oaire.awardURIhttps://digitalpro.inta.es/handle/123456789/1490
relation.isProjectOfPublication3a8b6e57-2574-4967-a3a1-4147efc5ee2f
relation.isProjectOfPublication18f93491-f3dd-4ec1-9fc1-25851087e49a
relation.isProjectOfPublicationafd59d7d-6b2b-493d-8a8c-679dd07513e3
relation.isProjectOfPublication.latestForDiscovery3a8b6e57-2574-4967-a3a1-4147efc5ee2f

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