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HIP 114328: A new refractory-poor and Li-poor solar twin

Melendez, Jorge; Schirbel, L; Monroe, Tala Wanda R.; Yong, David; Ramirez, Ivan; Asplund, Martin


Context. The standard solar model fails to predict the very low lithium abundance in the Sun, which is much lower than the proto-solar nebula (as measured in meteorites). This Li problem has been debated for decades, and it has been ascribed either to planet formation or to secular stellar depletion due to additional mixing below the convection zone, either during the pre-main sequence and thus possibly linked to planet formation, or additionally on secular time-scales during the main sequence....[Show more]

CollectionsANU Research Publications
Date published: 2014
Type: Journal article
Source: Astronomy and Astrophysics
DOI: 10.1051/0004-6361/201424172
Access Rights: Open Access


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