MILLER— PARALLAXES OF FIFTY STARS. 



129 



No. 36. B.D. -f 27°.339i. 2 2525. (ig^ 22^5; + 27° 7'.) 

 Mag. 7.5. Spectrum G. 



The measures are in longitude. This is a binary of long and un- 

 certain period. The components are separated by about ©".5. The 

 combined image of the components seemed sHghtly elongated. This 

 image was bisected in the measures. Russell gives a hypothetical 

 parallax of o".025 for this star. 



Solution: c = — o".i22. 



/A= + o".03i ± o".oo3. 

 TT = + o".oi3 dz o".oi3. 



p. e. unit weight, ± ".023. 



Comparison Stars. 



