SOLVED: Jeans Collapse In this problem, you will derive the Jeans mass, discussed in lecture: (Scharf: equation 2.16; Perryman: just after equation 10.1). Calculate the gravitational potential energy of a uniform spherical
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SOLVED: The final radius of a protostar R is a function of its mass and initial radius R: R = (GM)/(B+c*m) where p = 4.5 eV and e = 13.6 eV. From
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SOLVED: Building a star: a) The Jeans Mass of a spherical, uniform density gas cloud is (1/2)^(5kT/3) M. Derive the expression for the Jeans Radius, RJ. b) Assume uniform, non-rotating, Jeans collapse.
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