This transcription has been completed. Contact us with corrections.
[[start page]] [[preprinted]]30[[/preprinted]] [[underline]]February[[/underline]] 4, [[underline]]1896[[/underline]] Continuation of estimates of S Cephei from previous volume p. 153 Plate C8648 taken Dec. 20, 1895 V n.s. v < 11.00 10.80[[/ink]] m ns = .2 Plate C 8669 taken Dec. 22, 1895 V n.s. [[ink]] v < 11.94 11.64[[/ink]] V = .3 ^[[margin]] April 2,1896 [[/margin]] Plate C 8796 taken Jan. 30, 1896 V n.s. [[ink]]v < 11.74 11.64[[/ink]] V=.1 [[margin note]]April 2, 1896 [[/margin note]] Plate C8869 taken Feb. 20, 1896 v n.s. [[ink]]v < 11.00 10.80[[/ink]] n=.2 [[margin note]]April 2, 1896 [[/margin note]] Plate C8898 taken Feb. 24, 1896 V n.s. [[ink]]v < 11.26 10.96[[/ink]] n=.3 Plate C8899 taken Feb. 24, 1896 V n.s. [[ink]]v < 11.26 10.96[[/ink]] n=.3 Plate I 14409 taken Jan. 30, 1896 v op'? Any doubtful observation. What I have taken for V may be a defect in the plate Plate I 14738 taken March 27, 1896 V n.s. V=.2 Continued III p 135 [[end page]] [[start page]] [[preprinted]]31[[/preprinted]] [[underline]]Feb.[[/underline]] 5 , 1896. Annie J. Cannon obs. Estimates of the brightness of comparison stars to S Cygni Plate I 141, Taken Nov. 16. 1889. a | 4.7 b | 5.5 c | 5.4 d | [[strikethrough]]4[[/strikethrough]]5.6 e | 5.4 f | 6.1 g | 5.4 h | 7.2 k | 6.6 l | 6.9 m | 7.2 n | 7.9 o | 7.3 p | 7.8 q | 8.2 r | 8.4 s | 8.5 t | 8.9 Image blurred. Ft. star | 8.2 [[end page]]