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56

Friday, October 2 [strikethrough]7[\strikethrough]8, 1910

Sequence C1
Estimates of Orig. Nos. 3 and 9 selected as g and p by the Director and Mrs. F.

AM6619 | AC11230 | B38215 Sept. 29, 1907
d^[[3]]4(3) | d^[[3]]2[[strikethrough]]9[[/strikethrough]](3) | d^[[1]]0d^[[2]]
(3)1e | (3)1e | d^[[2]]7d^[[3]]
e2f | e2f | d^[[3]]0(3)
[[strikethrough]]K[[/strikethrough]] |   | (3)3e
   |   | e3f
k6l | k5l |   |
l2([[strikethrough]]3[[/strikethrough]][[9]]) | l0(9) | k5l
([[strikethrough]]3[[/strikethrough]][[9]])2(m) | 94m | l2(9)
   |   | (9)3m

[[new columns]]
MC599pc | A8196 Nov.14 1906 | I32017pc | d^[[2]]d^[[2]] |d^[[1]]6d^[[2]] | too ft | d^[[2]]7d^[[3]] | d^[[2]]0d^[[3]] |Reject prev. est
d^[[3]]2(3) | d^[[3]]-(3) | for d^[[2]]+d^[[3]
(3)3e | (3)-e |   |
e1f |   | [[new column]]I32017 star
   | k-l | d^[[1]]2d^[[2]]
[[new column]]MC599star [?] | l1(9) | d^[[2]]4d^[[3]]
k4l | (9)0m | d^[[3]]1(3)
l2(9) |   | (3)le
(9)2m |   |   |
   |   | l3(9)
   |   | 92m



57

Friday, October 28, 1910

Sequence C1
Examination of d^2 suspected of variability

B38209 Sept. 28, 1907 | I34359 | AM5173 Sept. 27, 1907
d1d^[[1]] | d0d^[[1]] | AC 8823 Oct. 2, 1907 of nearly same date as the 3B plates show the star normal
d^[[1]]0d^[[2]] | d^[[1]]1d^[[2]] | 
d^[[2]]8d^[[3]] | d^[[2]]5d^[[3]] |  
B 38214 Sept. 29, 1907 |   |
d1d^[[1]] | AW5258 |   |
d^[[1]]1d^[[2]] | d^[[1]]4d^[[2]] | AW4688 Nov. 13, 1906
d^[[2]]8d^[[3]] | d^[[2]]3d^[[3]] | Normal

AC979^[[5]] |[[strikethrough]] AC3705 [[/strikethrough]] | AC8008 Nov. 13, 1906
d^[[1]]3d^[[2]] | AM3425 | Normal
d^[[2]]5d^[[3]] | d^[[1]]4d^[[2]] |   |
   | d^[[?]]3d^[[3]] | AC8031 Nov. 19, 1906
AM6697 |   | Normal
d^[[1]]3d^[[2]] | AM3015 |   |
d^[[2]]4d^[[3]] | AC4188 |   |
   | AC2144 |   |
AC11264 | all the above show d62 normal
d^[[1]]4d^[[2]] | 
d^[[2]]5d^[[3]] 

No evidence of variation. The extreme faintness 
on A 8196 is probably due to a peculiarity of the image, though of course it might indicate a variable of the Algol type.

AM 6579
d^1 2 d^2
d^[[2]]5 d^[[3]] |