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Reappraising the Spite Lithium Plateau: Extremely Thin and Marginally Consistent with WMAP Data

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Meléndez, Jorge, Ramírez, Iván·2004·The Astrophysical Journal

Abstract

The lithium abundance in 62 halo dwarfs is determined from accurate equivalent widths reported in the literature and an improved infrared flux method temperature scale. The Li abundance of 41 plateau stars (those with T eff > 6000 K) is found to be independent of temperature and metallicity, with a star-to-star scatter of only 0.06 dex over a broad range of temperatures (6000 K < T eff < 6800 K) and metallicities (-3.4 < [Fe/H] < -1), thus imposing stringent constraints on depletion by mixing and production by Galactic chemical evolution. We find a mean Li plateau abundance of A Li = 2.37 dex ( 7 Li/H = 2.34 × 10 -10 ), which, considering errors of the order of 0.1 dex in the absolute abundance scale, is just in borderline agreement with the constraints imposed by the theory of primordial nucleosynthesis and Wilkinson Microwave Anisotropy Probe data (2.51 dex < A < 2.66 dex).

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Metadata

Authors
Meléndez, J., & Ramírez, I.
Venue
The Astrophysical Journal
Published
2004-09-27
Volume
615
Issue
1
Pages
L33-L36
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2069536714
Cited by
168
References
0
FWCI
9.06
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Reappraising the Spite Lithium Plateau: Extremely Thin and Marginally Consistent with WMAP Data. https://app.cochat.ai/papers/10.1086/425962
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Meléndez, J., & Ramírez, I. (2004). Reappraising the Spite Lithium Plateau: Extremely Thin and Marginally Consistent with WMAP Data. The Astrophysical Journal. https://doi.org/10.1086/425962

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