
This transcription has been completed. Contact us with corrections.
54 [[underlined]]May 18, 1904[[/underlined]] Exam. of plates for susp. var - 2° 3939 14^[[h]] 56^[[m]] 28.8^[[s]] - 2° 17.1 (9.6 max) 1855 Sp. Pec on I 31573 Cir 92 Sp. Pec Type IV. see I 31681 and I 28881 Cir 145 Dark Bands Type VI [[3 columned table]] |Plate|Date|Ex.| |---|---|---| |I 18179|June 1 1897| 17^[[m]]| |AM 1916|May 6 1903|60^[[m]]| |AC 2208|Jan 17 1902|90^[[m]]| |AC 2278|Feb 5 1902|60^[[m]]| |B 23574|July 19 1899|10^[[m]]| |B 29841|May 27 1902| 10^[[m]]| |B 29407|April 18 1920|10^[[m]]| |B 20311|Sept 14 1897|10^[[m]]| |B 23269|July 5 1899|13^[[m]]| |B 22546|April 8 1899|10^[[m]]| |B 25110|April 11 1900|10^[[m]]| |B 30462|July 26 1902|10^[[m]]| |B 21597|June 8 1898|10^[[m]]| |B 21162|April 11 1898|14^[[m]]| |B 18942|April 23 1897|10^[[m]]| |B 32171|July 13 1903|11^[[m]]| An examination of the above plates shows very little change in 2° 3939, except on B21162 where it is about 0.5 brighter than on the other plates. Not to be meas. of announced without further evidence. W.P.F. John C. Wolbach Library, Harvard-Smithsonian Center for Astrophysics. Provided by the NASA Astrophysics Data Systems