...Taking into account theapparent distribution of the stars in space, it is, however, more practicalto characterize the position of a star by its galactic longitude (l) andits galactic latitude (b)... 
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」
...The galactic longitude (l) is reckoned from the ascending node ofthe Milky Way on the equator, which is situated in the constellationAquila...
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」
...The squares GC and GD lie along the galactic equator (theMilky Way)...
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」
...Being probably many thousands of times more massive than the galactic stars, such a stellar missile would not be stopped by them, though its direction of flight might be altered...
Garrett Serviss 「Curiosities of the Sky」
...Instead of all moving one way, the galactic stars, as far as their movements can be inferred, are governed by local influences and conditions...
Garrett Serviss 「Curiosities of the Sky」
...Let us next count the number of stars visible in a powerful telescopein the region of the heavens around the galactic pole, now our zenith,and find the average number per square degree...
Simon Newcomb 「Side-lights on Astronomy and Kindred Fields of Popular Science」
...The galactic coordinates l and b are referred to the Milky Way(the Galaxy) as plane of reference...
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」
...But having ascertained later thatthe real position of the galactic plane requires a greater number of starsfor an accurate determination of its value...
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」
...Instead of giving the galactic longitude and latitude of a star wemay content ourselves with giving the galactic square in which the staris situated...
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」
...Eventually the position is given in galactic squares, as defined in ...
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」
...These components will be expressed in onecomponent (u0) parallel to the galactic plane, and one component (v0)perpendicular to it...
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」
...In the fourth column is the galactic square...
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」
...On the contrary we find only 6 in the galactic equator squaresand 12 in the other squares...
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」
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