Chapter 25: Problem 1
When quasi-stellar radio sources were first discovered and named, why were they called "quasi-stellar"?
Chapter 25: Problem 1
When quasi-stellar radio sources were first discovered and named, why were they called "quasi-stellar"?
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Get started for freeUse a telescope with an aperture of at least \(20 \mathrm{~cm}\) (8 in.) to observe the Seyfert Galaxy NGC 1068 (also known as M77). Located in the constellation Cetus (the Whale), this galaxy is most easily seen from September through January. The epoch 2000 coordinates are R.A. \(=2^{\mathrm{h}} 2.7^{\mathrm{m}}\) and Decl. \(=-0^{\circ} 01^{\prime}\). Sketch what you see. Is the galaxy's nucleus diffuse or starlike? How does this compare with other galaxies you have observed?
Calculate the Schwarzschild radius of a \(10^{9}\)-solar-mass black hole. How does your answer compare with the size of our solar system (given by the diameter of Pluto's orbit)?
How do astronomers know that quasars are located in galaxies? In what sorts of galaxies are they found?
. What is a blazar? What is unique about its spectrum? How is it related to other active galaxies?
What is a radio galaxy? What is a double radio source? Why do astronomers think these objects may be related to radioloud quasars?
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