W. S T R U F E. 



Epocha 



Tcmp. sid. 



Ainplif. 



Distantia 



Aiigiilus 



Magnitudines 





Ex hac relatione sequitur 













differentia in M. 



a— -1-17",114 inDecL h — 



-f 22",658 



quae ex formula p. CVIII evadunt 



-f 17, 119 





-\-22, 870 







Differentia 



0, 005 





0, 212. 



2780. EouuLEi 21. a — 



21^1l',2 



(T— 8°45'. P- 55 





1857,82 



2l''52' 



600 



2J27 



■X- 



185°5 



■X- 







In 12 annis inde ex 1825 nil fere in his stellis mutatum est. 



2900. 35PEGASI. 



a = 22^15',3. 



(V— 19°58'. P. 84. 



300. 









A et B. 









1837,82 



25\55' 



480 



A 



2,21 

 [ et C. 



180°1 







1837,82 





320 1 



57,50 1 



541,25 j 



1 





2917 a 



— 2'2!'2'ô' 



,8. d = 



: 52''58'. 



P. 101. 300. 





1837,75 



19^' 22' 



480 



// 



4,35 



69/7 







1837,75 



19 15 



480 



4,51 



70,8 







Médium 1837,75 







4,330 



70,25 







5019. Anonyma. 



a = 23''2l',7. 



(5 n: 4^19' 



P. 143. 





1837,82 



1 23^' 44' 



480 1 

 * 



10^80 



■X- 



1S5,°4 1 

 * 



1 





Observatio haec cum 



priorihus collata 



manifestât, inde ex 1828 per 9 



annos relaiionem inter has stellas mutationis expertem 



fuisse. 





