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56

October 16, 1905

Exam. of plates [[strikethrough]]for[[/strikethrough]]to det. var. if any in No. 5206 Nd? var? on I33313.
~9° 4911 R.A. 18^[[h]] 48.^[[m]][[strikethrough]]6[[/strikethrough]] Dec. -9° 8'.7 9.0 (1855).

[[three columned table]]|
|Plate|Date|Exp.|
|---|---|---|
|B 10163^[[(spectrum.)]]|Aug. 16 1893|60^[[m]]|
|I 21062|Aug. 15 1898|10|
|B 19203|May 25 1897|12|
|B 19089|May 12 1897|10|
|B 26206|Sept. 18 1900|12|
|B 23121|June 20 1899|10|
|B 23345|July 7 1899|10|
|B 2[[strikethrough]]6[[/strikethrough]]7619|June 7 1901|10|
|B 28363|Aug. 26 1901|10|
|B 28490|Sept. 7 1901|60|
|B 30042|June 13 1902|10|
|B 31736|May 7 1903|10|
|B 33496|April 23 1904|10|
|B 34405|July 21 1904|13|
|B 8470|   |   |
|B 12545|Nov. 13 1894|10|
|B 17556|Oct. 6 1896|12|
|B 18122|Nov. 30 1896|10|

An examination of the above plates fails to show any evidence of variation in the above star. The bright lines suspected may be due to defect, since [[strikethrough]]they[[/strikethrough]]an examination of [[strikethrough]]B[[/strikethrough]]I10163 fails to show any evidence of the spectrum being Md. It seems to be class K on that plate
W.PF.

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

Transcription Notes:
Upper text unclear.