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Gravitational Collapse

Stars - Introduction

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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

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Gravitational Collapse

Star Birth

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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Protostars | Landmarks of the ISM

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FORMATION AND EVOLUTION OF GALAXIES

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FORMATION AND EVOLUTION OF GALAXIES