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Isotopic abundances of silicon in four red giants
Authors:David L Lambert  Andrew McWilliam  Verne V Smith
Institution:(1) Department of Astronomy, University of Texas, Austin, Texas, U.S.A.
Abstract:High-resolution spectra near 4 mgrm of the four red giants—beta Peg,o 1 Ori, 10 Dra, and HR 1105—have been analysed to obtain estimates of the28Si/29Si and28Si/30Si abundance ratios. For betaPeg and the S star HR 1105, the28Si/29Si ratio is close to the solar ratio (28Si/29Si=20).29Si appears to be underabundant in the MS staro 1 Ori (28Si/29Si=40) and the M star 10 Dra (28Si/29Sisim53). The30Si isotope appears to be underabundant by, perhaps, about a factor of 2 in all four stars.
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