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The interstellar Li-7/Li-6 isotope ratio toward Zeta Ophiuchi and Zeta PerseiHigh S/N, high-resolution observations of the interstellar Li absorption lines toward the stars Zeta Ophiuchi and Zeta Persei are reported. Li I line profiles indicate the presence of both the Li-7 and Li-6 doublets in these two sightlines. Best-fit values for the interstellar Li-7/Li-6 isotope ratio are 6.8 (+1.4/-1.7) towards Zeta Ophiuchi and 5.5 (+ 1.3/-1.1) toward Zeta Persei. Measurement of 6.8 (+1.4/-1.7) for the interstellar Li-7/Li-6 isotope ratio towards Zeta Ophiuchi does not support the lower limit of 25 determined by Ferlet and Dennefeld (1984). The current value of the interstellar Li-7/Li-6 isotope ratio is the result of various lithium production and destruction processes involving stars, cosmic rays, and the big bang.
Document ID
19930054486
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Meyer, David M.
(Northwestern Univ. Evanston, IL, United States)
Hawkins, Isabel
(California Univ. Berkeley, United States)
Wright, Edward L.
(California Univ. Los Angeles, United States)
Date Acquired
August 16, 2013
Publication Date
June 1, 1993
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters
Volume: 409
Issue: 2
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
93A38483
Funding Number(s)
CONTRACT_GRANT: NSF AST-90-21641
CONTRACT_GRANT: NAS5-30180
CONTRACT_GRANT: NSF AST-90-23372
Distribution Limits
Public
Copyright
Other

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