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There Is A Mass Limit For A Star In The White Dwarf Phase, The Chandrasakhar Limit, Beyond Which The Star Can No Longer Support Itself Against Its Own Weight. This Mass Limit, In Terms Of Solar Mass, Is

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1. There Is A Mass Limit For A Star In The White Dwarf Phase, The Chandrasakhar Limit, Beyond Which The Star Can No Longer Support Itself Against Its Own Weight. This Mass Limit, In Terms Of Solar Mass, Is





 
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