The lithium-rotation connection in the newly discovered young stellar stream Psc-Eri (Meingast 1)

dc.contributor.authorBayo, Amelia
dc.contributor.authorArancibia Silva
dc.date.accessioned2021-08-25T21:05:52Z
dc.date.available2021-08-25T21:05:52Z
dc.date.issued2020
dc.description.abstractContext. As a fragile element, lithium is a sensitive probe of physical processes occurring in stellar interiors. Aims. We aim to investigate the relationship between lithium abundance and rotation rate in low-mass members of the newly discovered 125 Myr-old Psc–Eri stellar stream. Methods. We obtained high-resolution optical spectra and measured the equivalent width of the 607.8 nm LiI line for 40 members of the Psc–Eri stream, whose rotational periods have been previously derived. Results. We show that a tight correlation exists between the lithium content and rotation rate among the late-G to early-K-type stars of the Psc–Eri stream. Fast rotators are systematically Li rich, while slow rotators are Li depleted. This trend mimics that previously reported for the similar age Pleiades cluster. Conclusions. The lithium-rotation connection thus seems to be universal over a restricted effective temperature range for low-mass stars at or close to the zero-age main sequence, and does not depend on environmental conditions.en_ES
dc.identifier.doihttps://doi.org/10.1051/0004-6361/201937137e
dc.identifier.urihttp://repositoriobibliotecas.uv.cl/handle/uvscl/2273
dc.language.isoenen_ES
dc.publisherEuropean Southern Observatoryen_ES
dc.sourceAstronomy & Astrophysicsen_ES
dc.subjectSTARS: LOW-MASSen_ES
dc.subjectSTARS: PRE-MAIN SEQUENCEen_ES
dc.subjectSTARS: ABUNDANCESen_ES
dc.subjectSTARS: ROTATIONen_ES
dc.subjectOPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: PSC-ERIen_ES
dc.titleThe lithium-rotation connection in the newly discovered young stellar stream Psc-Eri (Meingast 1)en_ES
dc.typeArticuloen_ES
uv.catalogadorRCR DIBRAen_ES
uv.notageneralVarios autoresen_ES

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