The ____ depend(s) on the assumption that the mass of a galaxy or galactic cluster is large enough to keep moving matter bound to the main structure.
A) rotation curve method
B) velocity dispersion and cluster methods
C) Shapley-Curtis and Hubble methods
D) recessional velocity method
E) tangential velocity method
Correct Answer:
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Q34: Cepheid variables are useful in measuring the
Q35: The structure of most galaxies is most
Q36: The rotation curve of a galaxy is
Q37: The mass of a galaxy's central black
Q38: In general, _.
A) spiral galaxies are the
Q40: Because t he Hubble constant has a
Q41: Spiral galaxies are mostly found _.
A) in
Q42: At the longest look-back times, we see
Q43: The velocity dispersion method can be used
Q44: Rich galactic clusters _.
A) are rare, because
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