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Lecture 6: Jeans mass & length Anisotropies in 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 6: Jeans mass & length Anisotropies in CMB temperature  density ripples at the time of decoupling. These are the seeds that grow to form galaxies. - ppt download

Lecture 6: Jeans mass & length Anisotropies in 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 6: Jeans mass & length Anisotropies in 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