Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7505
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dc.contributor.authorDeepak-
dc.contributor.authorReddy, B. E-
dc.date.accessioned2020-11-27T12:54:43Z-
dc.date.available2020-11-27T12:54:43Z-
dc.date.issued2019-06-
dc.identifier.citationProceedings of the International Astronomical Union, Vol. 353, pp. 16-18en_US
dc.identifier.issn1743-9213-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/7505-
dc.descriptionRestricted Access © International Astronomical Union https://doi.org/10.1017/S1743921319008597en_US
dc.description.abstractHere, we explore the enrichment of Lithium in the Galaxy using a large sample of stars common among large spectroscopic surveys such as the GALAH and astrometric survey by the Gaia satellite. For this study we used about 60,000 low mass (M⩽ 2M⊙) dwarfs from the GALAH survey. Further, we discuss Li enrichment among giant stars based on a sample of 52,000 low mass giants, of which 335 are Li-rich with A(Li) ⩾ 1.80 ± 0.14 dex, culled from the GALAH survey. These low mass giants appears to be one of the promising source of Li enrichment in the Galaxy as their atmospheric Li can be added to the ISM through mass loss.en_US
dc.language.isoenen_US
dc.publisherCambridge University Pressen_US
dc.relation.ispartofseriesIAU Symposium No. 353;-
dc.subjectSurveys; Stars: evolutionen_US
dc.subjectGalaxy: evolutionen_US
dc.subjectGalaxy: abundancesen_US
dc.subjectNucleosynthesisen_US
dc.titleLithium enrichment in the Galaxy: A study using the GALAH and Gaia surveysen_US
dc.typeArticleen_US
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