Unformatted text preview: 1. Also ±nd the uncertainty in this M/L . Compare your value with the value of M/L ≃ 2 M ⊙ /L ⊙ expected for a “normal” stellar population. 3. Ryden problem 4.4 4. Ryden problem 4.5 Hint: to calculate the pressure you can either start with Ryden equation (4.32) or use the expression for the pressure of a gas of noninteracting particles with number density n , momentum p , and speed v : P = npv/ 3....
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This note was uploaded on 02/06/2012 for the course PHYSICS 444 taught by Professor Staff during the Fall '08 term at Rutgers.
 Fall '08
 Staff
 Current, Mass

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