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[[preprinted]] 62 [[/preprinted]] Feb. 13, 1907 [[checkmark]] C 16182 DC 2097 (1) Probably B8A Focus poor [[checkmark]] (2) K [[checkmark]] C 16638 DC 9646 Too poor Quality 2 [[checkmark]] C 16697 DC 9692 B9A? Very poor [[checkmark]] C 16702 DC 9692 Probably B8A 4026 quite strong [[end page]] [[start page]] [[preprinted]] 63 [[/preprinted]] [[underlined]] February 15, 1907 [[/underlined]] [[checkmark]] X 11191 S.M.P. 5886 F [[checkmark]] (2) A.G.C. 23073 Marked by W.P.F. as having spectrum similar to that of zeta Puppis. This spectrum is nearer like zeta Puppis than the spectrum of lambda Cephei is for in lambda Cephei, there are more lines between H beta and H gamma. Here as in zeta Puppis, only the two bright bands and H gamma are clearly seen, with a suspicion of 4471. H beta not clearly seen, probably due to faintness of the star. [[checkmark]] (3) A.G.C. 22962 A3F [[checkmark]] (4) A2F A.G.C. 23126 (5) Like epsilon Orionis between H beta & H gamma Too faint elsewhere. B Z.C. 16h 3761 = C.D.M. -38 degrees 11431 Not in A.G.C.