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24 August 19, 1905. Exam. of Plates for ident. of T Draconis for enl. for Mr Campbell. [[3 columned table]] | Plate| Date | Exp. | |------|-------------|--------| |I23165|July 14 1899|28^[[m]]|H. comp. br. |I32998sp.|April 8 1905|60^[[m]]| |I21506|Oct. 25 1898|10^[[m]]| |I20841|June 9 1898|15^[[m]]|H. comp. br. |I20498|March 14 1899|20^[[m]]| |I20736|April 21 1898|10^[[m]]| |I20657|April 7 1898|15^[[m]]| |I6744 |Aug. 17 1892|15^[[m]]| |I18767|Sept 13 1897|15^[[m]]| |I16443|Nov. 3 1896|14^[[m]]| |I13551|Sept. 30 1895|12^[[m]]| |I15795|Aug. 28 1896|11^[[m]]| |I9181 |Aug. 11 1893|19^[[m]]| |End I20783| | |H. comp. br. |I20608| | | |I29253|Sept. 10 1902|12^[[m]]| |I27442|Sept. 7 1901|15^[[m]]| |I18739|Sept. 9 1897|12^[[m]]| The above plates show very little variation (about 0.5 magn.) my the star which has been assumed to be J Draconis, count the specrive of this object is not fourth type. It may be Cl. Kur Ma. A faint star cloudy adjacent, but north shows a variation of at least 1.0 magnitude but it is much too faint on [[strikethrough]] these [[strikethrough]] plates and I32998 to show the class of specification. This may be J Draconis, eosphins fourth type star. If not, it is a star variable with P I [[illegible]] June 19, 1905