962 



In the following table I have combined my final results with those 

 obtained by other investigators according to the new reduction. 



Results for the solar motion. 



From the arrangement of these determinations into three groups, 

 it becomes clear that the ^-component certainly does not decrease 

 with decreasing magnitude of the stars. The equatorial movement 

 y^X^-\-Y* changes with the magnitude in a way that is to be 

 expected. Tiie results may be represented by the formula: 



