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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

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[[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.