Stellar Motions, With Special Reference to Motions Determined By Means of the Spectrograph

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We shall utilize only the t components of the observed proper motions. The results are condensed in Table XIX, in terms of visual magnitude. The proper-motion data were taken for the most part from Kapteyn's valuable lists in Piihli- cations of the Astronomical Laboratory at Groningen, No. 7, and the rest were collected from various sources. Stars whose t components of proper motion exceed 0".30 per annum were excluded. The numbers of stars of Secchi's Type I, Type II, Types I and II combined, ...the average t components, and the average residual radial velocities, are given in the table.
TABLE XIX Parallaxes by Magnitudes and Types From Radial Velocities and T Components of Proper Motion Type I Type II T\ 'PES I and II Vis. Mag.
11 7"™ F„, km.
n T,„ km.
km.
2.51-3.50 36 0".0148 9.2 50 0".0508 15.3 86 0".0357 12.7 3.51-4.50 76 .0279 8.8 150 .0545 15.3 226 .0455 13.1 4.51-5.50 58 .0266 8.6 162 .0352 14.0 220 .0329 12.5 7r„„ Type I "■„,, Type II 7r,„ Types laud II Vis. Mag.


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