How did Harlow Shapley use the period-luminosity relationship of RR Lyrae variables to determine the size of the Milky Way galaxy
A) He determined the proper motion of globular clusters in the outer disk of the galaxy.
B) He found the distances to individual variables free floating in the halo.
C) He found the distances to open clusters found throughout the disk of the galaxy.
D) He found the distances to globular clusters distributed about the center of the galaxy.
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Q18: Pulsating variable stars are useful in determining
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Q19: _ in other galaxies should contain luminous
Q20: The center of our galaxy lies in
Q21: The orbits of population I stars
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Q22: The energy source at the center of
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