The mass of a galaxy's central black hole is proportional to the mass of its _______________.
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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
Q46: One of the rare galaxies that is
Q47: A galaxy with randomly oriented elongated star
Q48: S0 galaxies have spiral arms, but little
Q49: Because the Hubble constant has a value
Q50: _ galaxies have star formation, but no
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