The Milky Way bulge

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dc.catalogadorjlo
dc.contributor.authorZoccali, Manuela
dc.contributor.authorValenti, Elena
dc.date.accessioned2025-03-12T19:21:30Z
dc.date.available2025-03-12T19:21:30Z
dc.date.issued2025
dc.description.abstractThis chapter reviews the three-dimensional structure, age, kinematics, and chemistry of the Milky Way (MW) region within ~2 kpc from its center (hereafter referred to as the 'bulge') from an observational perspective. While not exhaustive in citations, this review provides historical context and discusses the main controversies and limitations in the current consensus. The nuclear bulge region, within ∼200 pc from the Galactic center, has been excluded from this review. This very complex region, hosting dense molecular clouds and active star formation, would deserve a dedicated paper.
dc.fechaingreso.objetodigital2025-03-12
dc.fuente.origenORCID
dc.identifier.urihttps://doi.org/10.48550/arXiv.2412.01607
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/102540
dc.information.autorucInstituto de Astrofísica; Zoccali, Manuela; 0000-0002-5829-2267; 1003159
dc.language.isoen
dc.nota.accesocontenido completo
dc.revistaarXiv
dc.rightsacceso abierto
dc.titleThe Milky Way bulge
dc.typepreprint
sipa.codpersvinculados1003159
sipa.trazabilidadORCID;2025-03-03
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