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Gaia DR2 Distances to Planetary Nebulae

dc.contributor.authorGonzález Santamaría, I.
dc.contributor.authorManteiga, Minia
dc.contributor.authorManchado, Arturo
dc.contributor.authorUlla, Ana
dc.contributor.authorDafonte, Carlos
dc.date.accessioned2020-06-01T14:08:15Z
dc.date.available2020-06-01T14:08:15Z
dc.date.issued2020-04-01
dc.identifier.citationGonzález-Santamaría, I.; Manteiga, M.; Manchado, A.; Ulla, A.; Dafonte, C. Gaia DR2 Distances to Planetary Nebulae. Galaxies 2020, 8, 29. https://doi.org/10.3390/galaxies8020029es_ES
dc.identifier.issn2075-4434
dc.identifier.urihttp://hdl.handle.net/2183/25670
dc.description.abstract[Abstract] The aim of this work is to examine distances to planetary nebulae (PNe) together with other properties that were derived from them, using the astrometry of Gaia Data Release 2 (DR2). We were able to identify 1571 objects classified as PNe, for which we assumed distances calculated following a Bayesian statistical approach. From those objects, we selected a sample of PNe with good quality parallax measurements and distance derivations, which we called Golden Astrometry PNe sample (GAPN). In this paper we will review the physical properties of the stars and nebulae in this subsample of PNe.es_ES
dc.description.sponsorshipXunta de Galicia; ED431B 2018/42es_ES
dc.description.sponsorshipFunding from Spanish Ministry projects ESP2016-80079-C2-2-R, RTI2018-095076-BC22, Xunta de Galicia ED431B 2018/42, and AYA-2017-88254-P is acknowledged by the authors. M.M. thanks the Instituto de Astrofísica de Canarias for a visiting stay funded by the Severo Ochoa Excellence programme. IGS acknowledges financial support from the Spanish National Programme for the Promotion of Talent and its Employability grant BES-2017-083126 cofunded by the European Social Fund
dc.language.isoenges_ES
dc.publisherMDPI AGes_ES
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/ESP2016-80079-C2-2-R/ES/
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/RTI2018-095076-B-C22/ES/MINERIA DE DATOS DE GAIA PARA ESTUDIAR LA VIA LACTEA II
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/BES-2017-083126/ES/
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/AYA2017-88254-P/ES/NUCLEOSINTESIS Y PROCESOS MOLECULARES EN ESTRELLAS EVOLUCIONADAS: DE (RADIO)ISOTOPOS A NANOESTRUCTURAS MOLECULARES COMPLEJAS
dc.relation.urihttps://doi.org/10.3390/galaxies8020029es_ES
dc.rightsAtribución 4.0 International (CC BY 4.0)es_ES
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/*
dc.subjectPlanetary nebulaees_ES
dc.subjectGeneral starses_ES
dc.subjectDistances starses_ES
dc.subjectEvolutiones_ES
dc.subjectHertzsprung-Russell and colour–magnitude diagramses_ES
dc.subjectGalaxyes_ES
dc.subjectStellar contentes_ES
dc.titleGaia DR2 Distances to Planetary Nebulaees_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.accessinfo:eu-repo/semantics/openAccesses_ES
UDC.journalTitleGalaxieses_ES
UDC.volume8es_ES
UDC.issue2es_ES
UDC.startPage29es_ES
dc.identifier.doi10.3390/galaxies8020029


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