Chemical evolution of Mg isotopes versus the time variation of the fine structure constant

We show that the synthesis of (25,26)Mg at the base of the convective envelope in low-metallicity asymptotic giant branch stars can produce the isotopic ratios needed to explain the low-z subset (with z

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Veröffentlicht in:Physical review letters 2004-01, Vol.92 (4), p.041102-041102, Article 041102
Hauptverfasser: Ashenfelter, T, Mathews, Grant J, Olive, Keith A
Format: Artikel
Sprache:eng
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Zusammenfassung:We show that the synthesis of (25,26)Mg at the base of the convective envelope in low-metallicity asymptotic giant branch stars can produce the isotopic ratios needed to explain the low-z subset (with z
ISSN:0031-9007
1079-7114
DOI:10.1103/PhysRevLett.92.041102