The Gaia-ESO Survey: an extremely Li-rich giant in the globular cluster NGC1261

dc.contributor.authorBayo, Amelia
dc.date.accessioned2021-11-19T17:57:24Z
dc.date.available2021-11-19T17:57:24Z
dc.date.issued2020
dc.description.abstractLithium-rich stars in globular clusters are rare. Only 14 have been found so far, in different evolutionary phases from dwarfs to giants. Different mechanisms have been proposed to explain this enhancement, but it is still an open problem. Using spectra collected within the Gaia-ESO Survey, obtained with the GIRAFFE spectrograph at the ESO Very Large Telescope, we present the discovery of the first Li-rich star in the cluster NGC 1261, the second star known in the red giant branch bump phase. The star shows an extreme Li overabundance of A(Li)LTE = 3.92 ± 0.14, corresponding to A(Li)NLTE = 3.40 dex. We propose that the Li enhancement is caused by fresh Li production through an extra mixing process (sometimes referred to as cool bottom burning). Alternatively, it could be a pre-existing Li overabundance caused by mass-transfer from a red giant star; this mechanism does not enhance the barium abundance and thus we observe low barium. To unambiguously explain the Li enhancement in globular cluster stars, however, a reliable determination of the abundance of key species like Be, 6Li, 12C/13C, and several s-process elements is required, as well as detailed modelling of chromospheric activity indicators.en_ES
dc.facultadFacultad de Cienciasen_ES
dc.identifier.doihttps://doi.org/10.1051/0004-6361/202038435
dc.identifier.urihttp://repositoriobibliotecas.uv.cl/handle/uvscl/2679
dc.language.isoenen_ES
dc.publisherEuropean Southern Observatoryen_ES
dc.sourceAstronomy & Astrophysicsen_ES
dc.subjectSURVEYSen_ES
dc.subjectTECHNIQUES: SPECTROSCOPICen_ES
dc.subjectSTARS: CHEMICALLY PECULIARen_ES
dc.subjectGLOBULAR CLUSTERS: INDIVIDUAL: NGC 1261en_ES
dc.titleThe Gaia-ESO Survey: an extremely Li-rich giant in the globular cluster NGC1261en_ES
dc.typeArticuloen_ES
uv.catalogadorRCR DIBRAen_ES
uv.departamentoInstituto de Fisica y Astronomiaen_ES
uv.notageneralVarios autoresen_ES

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