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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
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