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Degenerate Electron Pressure limits contraction and
core
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temperature
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Stars with M < 0.08 MSun never burn
H (brown dwarfs)
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Stars with M <
0.4 MSun
never burn He (red dwarfs)
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Stars with M
< 4 MSun
never burn C (but do make red
giants)
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Stars with M > 4 MSun do burn
elements all the way to Fe
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What happens to these objects?
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Brown dwarfs never become bright sort of giant
version of Jupiter
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Red dwarfs have such long lives none have yet
exhausted H
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Red giants are related to white dwarfs
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Massive stars explode as supernova
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