The general Characteristics of the freqnencyfunction of stellar movements 49 



3 equations of the form 



V B" 013 I, + V #"o 31 h + V B" ni ? 3 = h q' 6 + / 5 2 "(1 - + 

 + h a'(2 - 2' - 2?' 2 + g' 5 ) + ? 7 g' 2 + / S (H - I2q' + 3g' 2 + 4g' 3 - g' 6 ), 

 given in the table 



h 



h 



h 



h 



h 



?o 



'7 



h 



+ 6.1830 



+ 0.9657 



+ 0.3210 



+ 8.3133 



+ 2.7977 



— 2.99(31 



— 2.7019 



+ 0.2773 



+ 0.965T 



+ 7.8570 



+ O.2080 



+16.5260 



4" 4.1 352 



— 5 2532 



— 6.0618 



4" 0.5065 



+ 0.3210 



+ 0.2080 



+ 2.5210 



+ 5.0679 



+ 1.0559 



— 1.2143 



— 1.3284 



4- 0.0551 



finally (i equations of the form 



= w 7 g' 6 + w„ î' 8 (l — g' 3 ) + w( 9 (2 — q — 2q- + q' b ) q 4- m 10 g' 2 + 

 -|l OTll (6 — 12 ? '+ 3g' 2 4-4g' 3 - 2 ' 6 ) 



and given by the table 



m j 



»? 2 



»J S 





"'5 



H 'c 



wv 7 







"'10 



tn n 



414.7440 



4" 0.0524 



4- 0.2500 



— 0.2337 



4- 2.0474 



4 0.5914 



4- 13.8829 



- 0.9798 



4- 0.7737 



— 4.1455 



— 0.0410 



4 0.0524 



4-14.5154 



4- 0.2520 



— 0.2341 



4 0.5911 



4- 2.1021 



4- 48 8587 



— 10.3444 



4- 9.6267 



—23.0590 



— 0.4800 



4 0.2500 



4- 0.2520 



4- 9.8900 



4- 0.0834 



4- 0.619(1 



4- 0.6190 



4 15.990(1 



— 3.2800 



4" 1.8801 



— 5.1859 



— 0.1000 



— 0.2337 



— 0.2342 



4 0.0834 



4- 4.1712 



4- 0.4981 



4- 0.4392 



4- 10.5492 



— 0.8894 



4 1 .1292 



— 4.72(11 



— 0.0336 



4" 2.0474 



4- 0.5911 



4-0.6196 



4" 0.4981 



4-6.0904 



4- 0.7602 



4 24.3770 



— 2.2405 



4- 1.7239 



— 6.0074 



— 0.1529 



4 0.5914 



4- 2.1024 



4- 0.(1190 



4" 0.4392 



4- 0.7602 



4" 6.0908 



4- 36.7593 



— 5.0750 



4" 4.6168 



— 13.5552 



— 0.4609 



Solving, we obtain as solutions 



V B& = fl« g' 6 + fl» 2 ' 3 (1 - g' 3 ) + Jff» (2 - q' - 2q* + g' 5 ) i + 

 + JET» q* + H™ (6 - I2q' + 3g' 2 + 4 : ,/ 3 4- g' 6 ) 



and we find: 



Lunds Universitets Årsskrift. N. F. Afd. 2. Bd 11. 



7 



