Abstract
WHEN engaged in the classification of stars, according to their photographic spectra, in 1893 2 I came across two sets of lines of unknown origin, one in the hottest stars, the other in stars of intermediate temperature.
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References
Phil. Trans., A, vol. 184, p. 675.
1st Note, Roy. Soe. Proc., vol. 58, p. 67; 2nd, ibid., vol. 58, p. 113; 3rd, ibid., vol. 58, p. 116; 4th, ibid., vol. 58, p. 192; 5th, ibid., vol. 58, p. 193; 6th, ibid., vol. 59, p. 4; 7th, ibid., vol. 59, p. 342.
Roy. Soc. Proc., vol. 60, p. 475; ibid., vol. 61, p. 148; ibid., vol. 61, p. 441.
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The Origins of the lines of α Cygni1. Nature 59, 342–343 (1899). https://doi.org/10.1038/059342d0
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DOI: https://doi.org/10.1038/059342d0
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