Bestimmung der Längendifferenz zwischen Pulkowa, Helsingfors etc. 45 



Juni 27. Helsingfors. Beobachter Järnefelt. 



Lage 

 des 

 Instr. 



m 



und Zeitsterne. 



К 



i 



a 



и 



о 



15.001 



h m s 



15 11 42 



— è 



9 



о / // 



-4-1 21 81.4 





о 



14.574 



13 



29 



—2 



9 



80.2 





о 



1 4.092 



15 



34 



—2 



8 



80.9 





о 



1JUU LI о 1 J. J. f 



20 



20.14 



—3.0 



[60.0] 



m s 

 20 58 02 



о 



12.333 



23 



7 



— 3 



0 



79.9 





w 



8.717 



26 



42 



-4-1 



6 



40.5 





w 



8.969 



27 



48 



-4-1 



6 



40.2 





w 



9.259 



29 



5 



4-1 



8 



39.9 





w 



Ô Bootis (11) 



34 



6.51 



-4-1 



7 



[60.6] 



57.77 



W 1 ) 



11.020 



36 



36.5 



-1-2. 



1 



40.4 





w 



11.256 



38 



1 



-4-2 



1 



40.9 





w 



(x Bootis (11) 



43 



8.46 



-+-2 



4 



[60.6] 



57.87 



w 



12.987 



45 



51 



-t-2 



7 



38.3 





0 



6.563 



49 



4 



—2 



2 



81.7 





0 



6.186 



50 



48.5 



—2 



4 



81.6 





0 



а Coronae (11) 



53 



25.71 



—2 



7 



[61.3] 



57.93 



0 



5.047 



56 



10.5 



—2 



5 



82.5 





Die Sterne unruhig; ohne Beleuchtung beobachtet. 



О 



12.240 



17 18 



13 



—2 



3 



-4-2 23 49.6 



о 



s Herculis (11) 



21 



39.08 



—2 



5 



[27.1] 



о 



11.281 



24 



41 



—2 



7 



48.6 



о 



10.998 



26 



35 



—2 



7 



46.6 



w 



9.765 



30 



23 



-h2 



0 



5.7 



w 



10.012 



33 



0 



-4-2 



2 



7.0 



w 



a Herculis (10) 



36 



42.20 



-t-2 



2 



[27.1] 



w 



10.962 



39 



20 



-4-2 



4 



4.7 



w 



11.155 



40 



58 



-h2 



5 



6.5 



w 



p Herculis (9}- 



44 



49.27 



-+-2 



4 



[27.1] 



w 



12.037 



48 



0 



-+-2 



9 



5.5 



w 



12.234 



49 



35 



-4-2 



8 



4.7 



0 



7.484 



54 



7 



— 1 



.9 



48.5 



0 



a Ophiuchi (11) 



57 



1.60 



—2 



.0 



[27.1] 



0 



6.858 



59 



41 



—2 



.2 



49.0 



0 



6.695 



18 



1.10 



—2 



.2 



48.5 



Die Sterne unruhig. Mit Feldbeleuchtung. 



К 



16 A 33 m 27 s 

 37 27 



K—P 



6 A 22'"50?87 

 51.47 



16 35 32 6 22 51.19 



К = 



к— T = 



К— p = 



к- f = 



16 Л 35'"32* 

 и- 20 46.81 

 6 24 0.75 

 8 14 25.15 



-20 58.00 



57.76 



57.66 



58.06 



К 



19 A 47'"58 S 

 52 59 



О W 

 u 9.991 9.987 



1 T 



ß — 2!70 



с -+- 0'709 — 



a Urs. min. 



h 



1 



m s 



10 53.1 



88° 36 



3.7 



ß Bootis 



14 



56 



59.94 



-+-40 54 



57.4 



д Bootis 



15 



10 



12.54 



н~33 48 



42.8 



[л Bootis 





19 



31.90 



-н37 50 



41.2 



a Coronae 





29 



7.73 



-4-27 9 



48.2 



К = 



15 



38 









и = 





•20 



57.90 







K—T - 



-t- 



20 



46.83 







K—p = 



6 



23 



51.40 







K-f = 



8 



14 



15.80 







О w 



(л 9.989 



ß — 2?75 



С -+- 0?724 — 



a Urs. min. 1 10 53.4 88 36 3.6 



e Herculis 16 55 16.55 -t-31 7 31.4 



а Herculis 17 8 39.94 ч- 14 32 43.6 



p Herculis 19 10.13 -4-37 16 19.3 



а Ophiuchi 28 50.66 -t-12 39 39.6 



К = 17 40 



и = — 21 57.87 



K—T= -+- 20 46.79 



К— p = 6 24 11.25 



К— f = 8 14 35.63 



K—P 



6 Л 23"'22!і4 

 22.96 



К = 19"47 m 18 J 



19 47 18 6 23 22.03 



К — T = -4- 20 46 . 73 

 К — p = 6 24 31 . 98 

 К— f = 8 14 56.35 



1) К angenommen 15 А 36 т 5б!5. 



