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11-1 Stars form from the gravitational collapse of immense clouds of interstellar gas and dust
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11-2 Most stars shine throughout their lives by converting hydrogen into helium through nuclear fusion
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11-3 Careful observations of star clusters provide insight into how a starâs mass influences how stars change over time
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11-4 Stars slowly become red giants
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11-5 Low-mass stars pulsate and eject planetary nebulae, leaving behind a white dwarf at the end of their life cycles
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