Cohen, Judith Gamora (1972) The Lithium Isotope Ratio in F and G Field Stars. Astrophysical Journal, 171 . pp. 71-77. ISSN 0004-637X. doi:10.1086/151259. https://resolver.caltech.edu/CaltechAUTHORS:20190529-103833996
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Abstract
A Fabry-Perot interferometer was used to obtain high-resolution profiles of the resonance line of Li i and λ6717.69 of Ca i in 14 bright F, G, and early K field stars. The observational data were fitted by computed theoretical line profiles to determine the rotational velocity, Li abundance, and Li isotope ratio for each star. The ^6Li/^7Li ratio was 0.1 or less in all the program stars
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Additional Information: | © 1972. The University of Chicago. Received 1971 June 21; revised 1971 August 16. I would like to thank Professor Guido Münch, who supervised this research, which was part of my doctoral thesis, and provided much assistance in making the observations. I thank Professor G. Herbig for the loan of his spectra and valuable conversations. I am grateful to Mr. Kurucz and Dr. Strom for the use of their computer programs. Financial support from the California Institute of Technology is gratefully acknowledged. | |||||||||
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DOI: | 10.1086/151259 | |||||||||
Record Number: | CaltechAUTHORS:20190529-103833996 | |||||||||
Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20190529-103833996 | |||||||||
Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
ID Code: | 95874 | |||||||||
Collection: | CaltechAUTHORS | |||||||||
Deposited By: | George Porter | |||||||||
Deposited On: | 29 May 2019 18:31 | |||||||||
Last Modified: | 16 Nov 2021 17:16 |
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