What makes dwarf stars so bright?
They are really, really hot.
To start, the dwarf stars you are talking about are only white dwarfs, which are extremely hot stars that are left over after a star goes nova. A white dwarf star's surface temperature is about ten times higher than it was before the star went nova.
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Because of their small size and high surface temperature, dwarf stars have a high luminosity-to-surface area ratio. Nuclear fusion in their cores is the primary source of their brightness; it releases energy in the form of heat and light when hydrogen is converted into helium.
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When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
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