5. The stars are more and more uniformly distributed over the
sphere as one goes from the helium stars through the hydrogen
and solar stars, to the red stars. The Class M stars show
little or no preference for the Milky Way. Of course, I am
speaking here of the brighter and nearer stars which we have
been able to study by means of the spectroscope, and not at all
of the faint stars which form the unstudied distant parts of
the Milky Way structure. The helium stars are young, their
motions are slow, and they have not wandered far from the place
of their birth. Not so with the older stars.
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