MILLER— PARALLAXES OF FIFTY STARS. 



127 



No. 35. B.D. + 38°.3466. 2 2481 (tt) ; Secchi 2 (tt^). (19'^ y^'.y; 

 38° 36'.) Mag. 8.0-8.0. ix = — o^o2Io; — o"io3. 



This is a triple star. We have designated the component A by tt, 

 and by tt^, the components B C, (Secchi 2), which are separated by 

 o".24, and whose combined image is sensibly round. In measuring 

 TT^ we bisected the combined image of the components. The proper 

 motion of A is not the same as that of B C. The measures are in 

 longitude. The same comparison field was used for both com- 

 ponents. Other parallaxes published are : 



Russell, (Hypothetical), -|-o".02i. 



Mitchell, (Photographic), tt -|- o".oi9 ± o.oio. 



ir^ -\- o" .04.6 ± O.OII. 



Table and Solutions for tt. 



