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A possible new interpretation of the results of $Δα/α$ from QSO absorption lines

The measurement of $Δα/α$ from the QSO absorption lines of Fe_II taken at two different redshifts (Quast et al, Levshakov et al) is compared with the result based on the 23 data points also obtained from VLT/UVES (Chand et al), to demonstrate that the apparent oscillatory time-dependence fitting the latter taken at face value is reinforced by the former claimed to be of much better accuracy.

preprint2005arXivOpen access
Yasunori Fujii
astro-ph
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Open access1 author1 topic
Imported metadata coverageMissing code, dataset, citation and institution fields are tracked without dominating the paper.Details
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Yasunori Fujii

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