UNIVERSE LL W/SAPLINGPLUS MULTI SEMESTER
UNIVERSE LL W/SAPLINGPLUS MULTI SEMESTER
11th Edition
ISBN: 9781319278670
Author: Freedman
Publisher: MAC HIGHER
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Chapter 24, Problem 4CC
To determine

The consequences if a quasar temporarily becomes brighter without much change in its mass. Assume the initial luminosity of the quasar to be right at the Eddington limit.

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What is the mechanism for the energy output of quasars?
Describe a quasar.
Suppose a quasar is shining with a luminosity L.  What is the approximate minimal mass of the black hole?  (If the black hole had a lower mass than this, the pressure in the material would overcome the gravity of the black hole and the material would be blown apart.) Give your answer in solar masses, in scientific notation to one significant figure (no decimal places).   Value: L = 1*10^12 Lsun​
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