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54

October 16, 1905.

Exam. of plates to det. var, if any in 
No. 5020 Sp. W Type Na Var? on I324[[strike through]]57[[/strike through]]^[[75]]
+31° 1388 Ra. 6^[[h]] 32^[[m]] 46^[[s]].7 Dec. +31° 35.1 8.1(1855,

[[three columned table]]
|I|   |   |
|I 33208|April 17 1903|14^[[m]]|
|I 5645|Feb. 15 1892|11^[[m]]|
|I 10765|March 7~ 1894|13|
|I 14697|March 24 1896|16|
|I 14641|March 13 1896|16|
|I 5561|Feb. 6 1892|13|
|I 6073|April 12 1892|10|
|I 5514|Feb. 4 1892|11|
|I 7842|Jan. 3 1893|15|
|I 7839|Jan. 3 1893|22|
|I 30264|April 1 1903|12|
|I 30249|March 29 1903|10|
|I 30351|April 21 1903|14|
|I 30344|April 20 1903|14|
|I 26070|Nov. 12 1900|10|
|I 8348|April 4 1893|12|
|I 8112|Feb. 27 1893|11|
|I 5412|Jan. 16 1892|17
|I 30320|April 18 1903|10|
|I 30365|April 24 1903|12|

An examination of the above plates shows a variation of about 0.7 magn. As this star is fourth type the change may be due to the photographic images but I think the variation is real. Measure? before announcing → W.P.F.
Star suspected of var. before. See note on I32475 (cover)
Later announced on Wendell's authority in Miss Cannon's 2nd cat. of variable stars as having range of 0.28 magn.

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

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