期刊
ASTROPHYSICAL JOURNAL LETTERS
卷 752, 期 1, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/2041-8205/752/1/L16
关键词
galaxies: dwarf; Local Group; stars: abundances
资金
- NASA [51256.01, NAS 5-26555]
- Space Telescope Science Institute
- NSF [AST 09-37525, AST-1010039]
- NSFC [10973015, 11061120454]
- Direct For Mathematical & Physical Scien
- Division Of Astronomical Sciences [0937523] Funding Source: National Science Foundation
- Division Of Astronomical Sciences
- Direct For Mathematical & Physical Scien [1010039] Funding Source: National Science Foundation
Stars destroy lithium (Li) in their normal evolution. The convective envelopes of evolved red giants reach temperatures of millions of kelvin, hot enough for the Li-7(p, alpha)He-4 reaction to burn Li efficiently. Only about 1% of first-ascent red giantsmore luminous than the luminosity function bump in the red giant branch exhibit A(Li) > 1.5. Nonetheless, Li-rich red giants do exist. We present 15 Li-rich red giants-14 of which are new discoveries-among a sample of 2054 red giants in Milky Way dwarf satellite galaxies. Our sample more than doubles the number of low-mass, metal-poor ([Fe/H] less than or similar to -0.7) Li-rich red giants, and it includes the most-metal-poor Li-enhanced star known ([Fe/H] = -2.82, A(Li)(NLTE) = 3.15). Because most of the stars have Li abundances larger than the universe's primordial value, the Li in these stars must have been created rather than saved from destruction. These Li-rich stars appear like other stars in the same galaxies in every measurable regard other than Li abundance. We consider the possibility that Li enrichment is a universal phase of evolution that affects all stars, and it seems rare only because it is brief.
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