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 |
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Hauptverfasser: | , , |
Format: | Artikel |
Sprache: | eng |
Online-Zugang: | Volltext |
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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 |
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ISSN: | 0031-9007 1079-7114 |
DOI: | 10.1103/PhysRevLett.92.041102 |