Separation of stellar populations by an evolving bar: implications for the bulge of the Milky Way

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dc.contributor.authorDebattista, Victor P.
dc.contributor.authorNess, Melissa
dc.contributor.authorGonzalez, Oscar A.
dc.contributor.authorFreeman, K.
dc.contributor.authorZoccali, Manuela
dc.contributor.authorMinniti, D.
dc.date.accessioned2021-05-22T01:11:00Z
dc.date.available2021-05-22T01:11:00Z
dc.date.issued2017
dc.format.extent25 páginas
dc.fuente.origenConveris
dc.identifier.doi10.1093/mnras/stx947
dc.identifier.eissn1365-2966
dc.identifier.issn0035-8711
dc.identifier.urihttps://doi.org/10.1093/mnras/stx947
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/59007
dc.identifier.wosidWOS:000406629100025
dc.issue.numeroNo. 2
dc.language.isoen
dc.nota.accesoContenido completo
dc.pagina.final1611
dc.pagina.inicio1587
dc.revistaMonthly Notices of the Royal Astronomical Societyes_ES
dc.rightsacceso abierto
dc.titleSeparation of stellar populations by an evolving bar: implications for the bulge of the Milky Wayes_ES
dc.typeartículo
dc.volumenVol. 469
sipa.codpersvinculados1003159
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