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[[start page]] [[preprinted]] 68 [[/preprinted]] October 3, 1904 -15 [[symbol - degree]] 4905 continued Plate AM 153 [[symbol - check]] Sept. 21, 1899 942 b1v 952 9 [[strikethrough]] 52 [[/strikethrough]] 47 9 [[strikethrough]] 52 [[/strikethrough]] 50 [[strikethrough]] 00 [[/ strikethrough]] [[strikethrough]] 00 [[strikethrough]] 02 [[underlined]] 03 [[/underlined]] 9.[[strikethrough]] 52 [[/strikethrough]] 47 v2c 9.[[strikethrough]] 72 [[/strikethrough]] 67 [[end page]] [[start page]] [[preprinted]] 69 [[/preprinted]] [[underlined]] October 4, 1904 [[/underlined]] -15 [[symbol - degree]] 4905 continued Plate B 29858 May 27, 1902 9.[[strikethrough]] 94 [[/strikethrough]] 89 d4v 10.[[strikethrough]] 34 [[/strikethrough]] 29 10.[[strikethrough]] 44 [[/strikethrough]] 39 10.[[strikethrough]] 39 [[/strikethrough]] 34 [[underlined]] 05 [[/underlined]] 05 10.[[strikethrough]] 44 [[/strikethrough]] 39 v1e 10.[[strikethrough]] 54 [[/strikethrough]] 49 Plate B 11363 June 2, 1904 Preceding spectra 9.89 d3v 10.19, 1029 10.24 [[underlined]] 05 [[/underlined]] ,05 v2e 10.49 The variable is [[strikethrough]] certainly [[/strikethrough]] probably very faint, but slightly brighter than e. There is an appearance as if another spectrum more superposed on d, but as the relative brightness of the stars of the sequence seems to be normal, d has been used in the comparison Middle spectra [[strikethrough]] c3v [[/strikethrough]] 9.67 c1v 9.77, 9.79 9.78 [[underlined]] 01 [[/underlined]] , 01 [[strikethrough]] v0d [[/strikethrough]] v1d 9.89 [[strikethrough]] v4l [[/strikethrough]] [[strikethrough]] Last [[/strikethrough]] [[?]] spectra 9.42 b3v 9.72, 9.67, 9.79, 9.73 [[underlined]] 01 [[/underlined]] , [[underlined]] 06 [[/underlined]] , 06 v0c 9.67 v1d 9.89 Evidently the spectra on the following side of the plate were taken first, if the successive images were caused by the stopping of the dark between [[strikethrough]] the [[/strikethrough]] times. [[strikethrough]] of their [[/strikethrough]] ([[?]]) [[end page]]