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6. (a) Calculate the Eddington Luminosity of Sgr A* and Cygnus X1. (b) Now calculate the Absolute (bolometric) Magnitude of both objects. (c) At what

6. (a) Calculate the Eddington Luminosity of Sgr A* and Cygnus X1. (b) Now calculate the Absolute (bolometric) Magnitude of both objects. (c) At what distance would black holes of these masses accreting at the Eddington limit have the same apparent magnitude?

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