Related articles:
Solar mass
Type Ia supernova
White dwarf
Subrahmanyan Chandrasekhar
Degenerate matter
Neutron star
Black hole
Arthur Stanley Eddington
Key terms:
mass
star
limit
core
energy
kg
electron
chandrasekhar
supernova
white dwarf
equation
fusion
radius
collapse
value
nuclei
density
giving
fermi gas
frac
rise
approximately
stoner
relativistic
increases
elements
pauli
becomes
physicist
matter
arthur
temperature
eddington
maximum
neutron
massive
physics
solar mass
degenerate
observed
compression
equation of state
black hole
type ia supernova
chandrasekhar limit
gravitational
nuclear fusion
nonrelativistic
electron degeneracy pressure
model white dwarf
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