A revised view of the Canis Major stellar overdensity with DECam and Gaia: new evidence of a stellar warp of blue stars

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dc.catalogadorkjc
dc.contributor.authorJulio A Carballo-Bello
dc.contributor.authorDavid Martínez-Delgado
dc.contributor.authorJesús M Corral-Santana
dc.contributor.authorEmilio J Alfaro
dc.contributor.authorCamila Navarrete
dc.contributor.authorA Katherina Vivas
dc.contributor.authorCatelan , Marcio
dc.date.accessioned2024-03-04T17:01:45Z
dc.date.available2024-03-04T17:01:45Z
dc.date.issued2020
dc.fuente.origenORCID
dc.identifier.doi10.1093/mnras/staa2655
dc.identifier.urihttps://doi.org/10.1093/mnras/staa2655
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/83700
dc.information.autorucInstituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556
dc.language.isoen
dc.rightsacceso abierto
dc.titleA revised view of the Canis Major stellar overdensity with DECam and Gaia: new evidence of a stellar warp of blue stars
dc.typeartículo
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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