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145

[[underlined]] October 26, 1896 [[/underlined]]

Exam of photographs to determine variation if any in zeta^[[1]] or zeta^[[2]] Doradus for Stanley Williams. See letter of Oct. 13, 1896.
 
Plates. ^[[A.G.C. 7579 7581} 6 12.0 - 65 30{7 1/2 8 (1900)]]                                    
[[4 Column Table]]
--- | --- | --- | --- 
chart | B 4503 | Taken | Oct. 22 1889
chart | B 5720 | Taken | Sept. 12 1890
Spectrum | B 5745 | Taken | Sept. 16 1890
chart | B 7043 | Taken | Oct. 8 189[[strikethrough]]2[[/strikethrough]]1
chart | B 7063 | Taken | Oct. 21 1891
chart | B 7065 | Taken | Oct. 22 1891
chart | B 7092 | Taken | Oct. [[strikethrough]]27[[/strikethrough]]28 1891
chart | B 8870 | Taken | Dec. 12 1892
chart | B 8872 | Taken | Dec. 13 1893
chart | B 10208 | Taken | Aug. 21 1893
chart | B 10900 | Taken | April. 16 1894
chart | B 10914 | Taken | April. 17 1894
Spectrum | B 12108 | Taken | Sept. 10 1894
chart | B 12705 | Taken | Dec. 13 1894
Spectrum | B 12762 | Taken | Dec. 18 1894
chart | B 14824 | Taken | Oct. 12 1895
chart | B 14950 | Taken | Oct. 24 1895
chart | B 15040 | Taken | Oct. 30 1895
chart | B 15068 | Taken | Oct. 31 1895
Spectrum | B 15147 | Taken | Nov. 13 1895

zeta^2 Doradus is fainter than zeta^1 Doradus and brighter than [[strikethrough]] the combined light of[[/strikethrough]] A.G.C. 7579 [[strikethrough]] 7581[[/strikethrough]] 7 1/4 magn on all of the plates given above.  
Exam. Oct. 26, 1896.

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

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