...In and around the Sagittarius region the intermingling of nebulæ and galactic star clouds and clusters is particularly remarkable... 
Garrett Serviss 「Curiosities of the Sky」
...The richest galactic regions in the Northern Hemisphere are found inPerseus, Cygnus, and Aquila...
Thomas Orchard 「The Astronomy of Milton's 'Paradise Lost'」
...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 latitude (b) gives the angular distance of the starfrom the Galaxy...
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」
...Arranging the constellations according to theirgalactic longitude we find north of the galactic equator (in the C-squares)the constellations:—...
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」
...It lies in the square GD7 and its galactic coordinates are seenin the 5th and 6th columns...
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」
...In the fourth column is the galactic square...
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」
...It may be, as some astronomers hold, that most of the galactic stars are much smaller than the sun, so that their faintness is not due entirely to the effect of distance...
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」
...Consequently, the galactic stars areregarded as his peers or superiors in magnitude and brilliancy...
Thomas Orchard 「The Astronomy of Milton's 'Paradise Lost'」
...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」
...Twelvelie north of the galactic plane, between 0° and 30° galactic latitude, andare designated GC1, GC2, ...
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」
...A large radial velocity seems thereforeto be a galactic phenomenon and to be correlated to a great distancefrom us...
Carl Vilhelm Ludvig Charlier 「Lectures on Stellar Statistics」
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