Abstract
THE peculiar A star HR465 is a spectrum variable1. Considerable attention2,3 has been given to the spectra of this star obtained by W. P. Bidelman during 1960–61, when the lines of the rare earth elements attained their maximum intensity; Bidelman has kindly placed this material at our disposal. Among the remarkable aspects of the HR465 spectrum is the fact that it is the only star for which a firm statistical basis exists for the identification of uranium4.
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References
Aller, M. F., Astr. Astrophys, 19, 248–260 (1972).
Hartoog, M. R., Cowley, C. R., and Cowley, A. P., Astrophys. J., 182, 847–858 (1973).
Ohnishi, T., Nature, 249, 532–533 (1974).
Cowley, C. R., and Hartoog, M. R., Astrophys. J. Lett., 178, L9–L10 (1972).
Cowley, C. R., Hartoog, M. R., and Cowley, A. P., Astrophys. J., 194, 343–354 (1974).
Meggers, W. F., Corliss, C. H., and Scribner, B. F., US Nat. Bur. Std Monogr., No. 145 (1975).
Corliss, C. H., and Bozman, W. R., US Nat. Bur. Std Monogr., No. 53 (1962).
Cowley, C. R., Hartoog, M. R., Aller, M. F., and Cowley, A. P., Astrophys. J., 183, 127–131 (1973).
Martin, W. C., Hagen, L., Reader, J., and Sugar, J., J. Phys. Chem. Ref. Data, 3, 771–780 (1974).
Michaud, G., Astrophys. J., 160, 641–657 (1970).
Havnes, O., and Conti, P. S., Astr. Astrophys., 14, 1–11 (1971).
Cameron, A. G. W., Sci. Rev., 15, 121–146 (1970).
Blake, J. B., and Schramm, D. N., Astrophys Space Sci., 30, 275–290 (1974).
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COWLEY, C., ALLEN, M. & AIKMAN, G. Thorium in the spectrum of HR465. Nature 258, 311 (1975). https://doi.org/10.1038/258311a0
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DOI: https://doi.org/10.1038/258311a0


