ESSN COSMIC PERSP ALC&MOD MSTG/&STARRY 8
ESSN COSMIC PERSP ALC&MOD MSTG/&STARRY 8
8th Edition
ISBN: 9780137437979
Author: Bennett
Publisher: PEARSON
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Chapter 16, Problem 56EAP
To determine

The data in below figure shows the Doppler shifts of emission lines from gas at a distance of 60 light-years from the center of the galaxy M87. Let us assume that the emission lines are observed from gas 30 light-years from the center. How would once expect the Doppler shifts of those lines to be different, supposing that the gas is orbiting a supermassive black hole. Also, what about the gas at 120 light-years from the center?

  ESSN COSMIC PERSP ALC&MOD MSTG/&STARRY 8, Chapter 16, Problem 56EAP

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ESSN COSMIC PERSP ALC&MOD MSTG/&STARRY 8

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