GRAVITATIONAL INSTABILITY IN RADIATION PRESSUREYDOMINATED BACKGROUNDS
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Lecture 6: Jeans mass & length Anisotropies in the CMB temperature density ripples at the time of decoupling. These are the seeds that grow to form galaxies. - ppt download
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Lecture Seven: Galaxy Formation
Lecture 6: Jeans mass & length Anisotropies in the CMB temperature density ripples at the time of decoupling. These are the seeds that grow to form galaxies. - ppt download
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Star formation: the Jeans criterion
Star formation: the Jeans criterion
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