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55

October 16, 1905.

Exam. of plates to det. var, if any in 
No 5122 [[strikethrough]] Type III [[/strikethrough]] Md? Var? in I33088
+35° 2792 16^[[h]] 7^[[m s]] +35° 49'.0'= 94 (1855),

[[three columned table]]
|Plate|Date|Ex.|
|---|---|---|
|I 1673|Aug. 25 1890|10^[[m]]|
|I 21715|Sept. 1 1900|10^[[m]]|
|I 26947|May 3 1901|10^[[m]]|
|I 8788|July 16 1893|10^[[m]]|
|I 6521|July 7 1892|11^[[m]]|
|I 3955|Aug. 8 1891|10|
|I 22813|April 29 1899|15|
|I 22784|April 27 1899|16|
|I 21230|Sept. 21 1898|9|
|I 6527|July 8 1892|11|
|I 8805|July 19 1893|10|
|I 25714|Sept. 1 1900|10|
|I 21311|Oct. 3 1898|11|
|I 24862|March 16 1900|13|
|I 15651|Aug. 10 1896|10|
|I 18282|June 25 1897|10|
|I 18292|June 26 1897|15|
|I 16063|Sept. 30 1896|10|

An examination of the above plates shows a variation of about 0.7 magn. in this star. It gives every evidence of being a real variation in the star. Measure before announcing. 
W.P.F

John G. Wolbach Library, Harvard-Smithsonian Center for Astrophysics · Provided by the NASA Astrophysics Data System