Bahnbestimmiing des Planeten (258) Tyclie. 



95 



I, 



No. 



Beobachter 



Datum 



4. 



5- 



6. 

 r 



7. 

 Reduct. 



9. 



z 



10, 

 Ext. 



1 1. 



12. 

 a 



2 



4 



5 

 6 



7 

 8 



9 



10 

 II 

 12 



13 

 14 



15 

 16 



17 

 18 



19 

 20 

 21 



22 



23 

 24 



25 

 26 



27 

 28 



29 

 30 

 31 

 32 



34 



35 



36 



40 



41 

 42 



43 

 44 



45 

 46 



47 

 48 



49 



E.Lutlier 

 Big'ourdan 

 Millosevich 



U. Luther 



Stephan 



W. Luther 



Knorre 



R. Luther 



Millosevich 



Knorre 



J. Palisa 



Knorre 



Millosevich 



W. Luther 



)i 



» 



Millosevich 



J. Palisa 



C.H. F. Peters 



W. Luther 

 R. Luther 



Cerulli 

 W. Luther 

 R. Luther 

 W. Luther 

 R. Luther 

 W. Luther 



)) 

 R. Luther 

 W. Luther 



R. Luther 



Millosevich 

 W. Luther 



R. Luther 

 W. Luther 



W. Luther 

 R. Luther 

 W. Luther 



» 

 R> Luther 



W. Luther 

 Millosevich 



Schorr 

 W. Luther 



Schorr 



[886 Mai 



Juni 



Juli 



1887 Juli 



Aug. 



10 

 10 

 20 

 21 

 21 

 21 



23 



28 



I 



4 



5 

 6 



7 



22 



iS 

 21 



23 

 00 



22 

 24 

 26 

 26 

 Sept. 10 

 16 

 ^ Nov. 15 

 17 

 17 



1889 ,Jan. 28 

 Febr. 4 



1890 April 



1891 Juli 



15 



26 

 28 

 •^i 



Aug. 



1892 Dec. 23 



1893 ,Jan. 6 



10 

 10 



1894 März 25 



II. 3 



0.297 



0.474 



12.0 



0.297 



0.474 



II. 5 



0.297 



0.473 



12.0 



0.298 



0.473 



II. 3 



0.298 



0.473 



11-5 



0.298 



0.473 



11,6 



0.298 



0.473 



12.3 



0.306 



0.471 



II-5 



0.307 



0.471 



II. 8 



0.307 



0.471 



12.5 



0.307 



0.471 



II. 7 



0.309 



0.470 



12.5 



0.315 



0.469 



12.3 



0.321 



0.468 



11-5 



0.326 



0.467 



12.0 



0.328 



0.467 



12.0 



0.329 



0.467 



12.5 



0.331 



0.467 



12.3 



0.335 



0.466 



13.0 



0.381 



0.460 



13.0 



0.420 



0.4S5 



13.0 



0.422 



0.455 



10.9 



0. 151 



0.329 



10.8 



0.142 



0.328 



II .0 



0.136 



0.328 



9.8 



0.062 



0.322 



9.7 



0.062 



0.322 



9.8 



0.059 



0.322 



9-5 



0.056 



0.321 



9.9 



0.056 



0.321 



9.7 



0.044 



0.319 



9.7 



0.044 



0.319 



II. 7 



0. 180 



0.318 



II. 5 



0. 186 



0.319 



II. 5 



o.i85 



0.319 



12.0 



0.2S8 



0.459 



12.4 



0. 291 



0.461 



"■5 



0.321 



0.491 



II. 5 



0.321 



0.491 



10.2 



0. 112 



0.353 



10.5 



0. HO 



0.352 



10.6 



0. 109 



0.351 



II .0 



0. 108 



0.350 



10.5 



0. 1 10 



0.347 



II. 4 



0.241 



0.423 



11-5 



0.241 



0.428 



II. 6 



0.243 



0.429 



II. 4 



0.243 



0.429 



12.3 



0.334 



0.498 



— o. 72 



— o. 72 



— o. 72 



— 0.72 



— o. 72 



— o. 72 



— o. 72 



— 0.75 



— o. 76 



— 0.76 



— 0.76 

 — • 0.76 



— 0.79 



— 0.81 



— 0.83 



— 0.84 



— o . 85 



— O.S6 



— 0.87 



— 1 .07 



— 1.24 



— 1.25 



+ 0.73 

 + 0.78 



+ 0.81 



4-1.21 



-}- I ■ 21 



+ 1.23 



+ 1.25 



+ 1.25 



+ 1.32 



+ 1.32 



+ 0.64 



+ 0.61 



+ 0.61 



— • o. 60 



— 0.63 



— 0.93 



— 0.93 



+"o.8i 

 + 0.82 

 + 0.83 

 + 0.84 

 + 0.S5 



— 0.19 



— 0.21 



— 0.23 



— 0.23 



— 1 . 03 



Bei den Beobachtungen No. 26, 28 bis 31 kommt die Extinction in 



Fortfall, weil diese Schätzungen durch Vergleichu 



0.58 

 1.28 

 0.78 

 1.28 

 0.58 

 0.78 

 0.88 



1-55 



0.74 



04 



74 



94 



71 



49 



0.67 



.16 



• 15 

 .64 

 .43 

 .93 

 .76 



• 75 



.63 



.58 



.81 



.01 



0.91 



1.03 



0.75 



.15 

 ,02 

 ,02 

 .34 



1 1 



2 . II 



1 .40 



1.77 



0.57 

 0.57 



1 .01 

 1.32 



1-43 

 1.84 



1-35 



1 .21 

 1 .29 

 1-37 

 1.17 



1 . 27 



61° 



58 



52 



51 

 60 



54 



63 

 62 



59 

 50 

 62 



58 

 61 



48 

 72 

 73 

 67 

 70 

 75 

 70 

 71 

 71 



55 

 47 

 39 



52 



47 

 68 



55 

 53 



45 

 56 



62 

 63 



48 

 46 

 50 

 58 

 48 



55 

 42 



54 

 60 



o. 24 

 o. 19 



O. II 



o. 10 

 0.22 

 o. 13 



0.28 



0.26 

 o. 20 

 0.09 

 0.26 

 o 19 

 0.24 

 0,07 



0.53 

 0.57 

 0.37 

 0.45 

 0.65 



0.45 

 0.49 

 0.49 



o. 14 

 0.07 



0,03 



O. II 



0.07 

 0.40 

 o. 14 

 0.12 



0.05 



o. 16 



0.26 



0.28 



0.07 

 o 06 

 o 09 

 o. 19 

 0.07 



o 14 

 0.04 



0.13 



0.22 



34 

 09 

 67 

 18 

 36 



65 

 60 



29 



54 

 95 

 48 



75 

 47 

 42 

 14 

 59 

 78 

 19 

 78 

 48 

 27 

 26 



49 

 51 



78 



Ol 



80 

 03 

 75 

 15 

 02 



95 

 94 

 97 

 99 



35 

 61 



94 

 26 



4^ 



4 



5 



5 



5 



5 



5 



9 



9 



9 



9 



o 



2 



3 



4 



4 



4 



5 



5 



9 

 21 

 21 



24 

 23 

 23 

 13 

 13 

 13 



12 

 12 



9 



9 



26 



27 

 27 



10 



8 



o 

 o 



1 1 



1 1 



34 j II 

 65 I II 

 28 I I -, 



10 

 10 



07 



25 



24 ! 10 



95 10 



10.99 3 



lg des Planeten mit 



Diirclimusterungssternen nach der Stnfenschätzungsmethode erlangt sind. 



