RR Lyrae stars as tracers of halo substructures

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dc.catalogadormas
dc.contributor.authorDuffau, Sonia
dc.contributor.authorVivas, A. Katherina
dc.contributor.authorNavarrete, Camila
dc.contributor.authorCarballo-Bello, Julio
dc.contributor.authorHajdu, Gergel
dc.contributor.authorCatelan, Marcio
dc.date.accessioned2024-02-02T13:58:36Z
dc.date.available2024-02-02T13:58:36Z
dc.date.issued2017
dc.description.abstractThree RR Lyrae overdensity candidates in the southern sky have been studied using low resolution spectra obtained with the Goodman spectrograph at SOAR. We search for unidentified velocity peaks indicative of the possible presence of streams within the overdensities. Our results suggest that all three overdensities present an excess of radial velocity signal at high mean radial velocities which cannot be explained as a contribution from any known Galactic component....
dc.fechaingreso.objetodigital2024-05-29
dc.fuente.origenORCID
dc.identifier.doi10.1051/epjconf/201715202013
dc.identifier.urihttps://doi.org/10.1051/epjconf/201715202013
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/81203
dc.identifier.wosidWOS:000426610100040
dc.information.autorucInstituto de Astrofísica; Catelan , Marcio; 0000-0001-6003-8877; 1001556
dc.language.isoen
dc.nota.accesoContenido completo
dc.rightsacceso abierto
dc.titleRR Lyrae stars as tracers of halo substructures
dc.typecomunicación de congreso
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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