Whiting 1: Confirmation of its accretion by the Milky Way

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dc.catalogadorgjm
dc.contributor.authorCarballo-Bello, Julio A.
dc.contributor.authorCorral-Santana, Jesús M.
dc.contributor.authorMartínez-Delgado, David
dc.contributor.authorSollima, Antonio
dc.contributor.authorMuñoz, Ricardo R.
dc.contributor.authorDuffau, Sonia
dc.contributor.authorCatelan, Marcio
dc.date.accessioned2024-02-02T13:58:36Z
dc.date.available2024-02-02T13:58:36Z
dc.date.issued2017
dc.description.abstractWe investigate the association of Whiting 1 with the Sagittarius tidal stream by obtaining radial velocities for a sample of 101 stars observed with VIMOS. Our results reveal the presence of a component of the Sagittarius tidal stream with a radial velocity - and distance - compatible with that of the globular cluster. Therefore, we conclude that Whiting1 was formed in the interior of the Sagittarius dwarf spheroidal galaxy and later accreted by the Milky Way. In addition, our data also reveal the detection for the first time of an ancient wrap of the Sagittarius tidal stream along the same line-of-sight and at the same heliocentric distance....
dc.fechaingreso.objetodigital2024-05-23
dc.fuente.origenORCID
dc.identifier.doi10.1051/epjconf/201715204006
dc.identifier.urihttps://doi.org/10.1051/epjconf/201715204006
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/81205
dc.information.autorucInstituto de Astrofísica; Catelan, Marcio; 0000-0001-6003-8877; 1001556
dc.language.isoen
dc.nota.accesoContenido completo
dc.rightsacceso abierto
dc.titleWhiting 1: Confirmation of its accretion by the Milky Way
dc.typecomunicación de congreso
sipa.codpersvinculados1001556
sipa.trazabilidadORCID;2024-01-22
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