Most lithium-rich low-mass evolved stars revealed as red clump stars by asteroseismology and spectro...
Most lithium-rich low-mass evolved stars revealed as red clump stars by asteroseismology and spectroscopy
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Yan, Hong-Liang , Zhou, Yu-Tao , Zhang, Xianfei , Li, Yaguang , Gao, Qi , Shi, Jian-Rong , Zhao, Gang , Aoki, Wako , Matsuno, Tadafumi , Li, Yan , Xu, Xiao-Dong , Li, Haining , Wu, Ya-Qian , Jin, Meng-Qi , Mosser, Benoit , Bi, Shao-Lan , Fu, Jian-Ning , Pan, Kaike , Suda, Takuma , Liu, Yu-Juan , Zhao, Jing-Kun and Liang, Xi-Long
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London: Nature Publishing Group UK
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English
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London: Nature Publishing Group UK
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Lithium has confused scientists for decades at almost every scale of the universe. Lithium-rich giants are peculiar stars with lithium abundances greater than model prediction. A large fraction of lithium-rich low-mass evolved stars are traditionally supposed to be red giant branch (RGB) stars. Recent studies, however, report that red clump (RC) st...
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Most lithium-rich low-mass evolved stars revealed as red clump stars by asteroseismology and spectroscopy
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TN_cdi_proquest_journals_2477821715
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2477821715
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ISSN
2397-3366
E-ISSN
2397-3366
DOI
10.1038/s41550-020-01217-8
