Hoyle discovered that one theory about these objects does not apply in non-uniformly rotating examples. Eddington predicted the first observed gravitational redshift from an object of this kind, initially as a way to discredit Öpik's measurement of its density. These stars are supported by Fermi pressure. Found in the lower left of a standard Hertzsprung-Russell diagram, these stars are generally bounded in mass by a quantity equal to about 1.44 solar masses and known as the Chandrasekhar limit. For 10 points, name this class of stars, the endp
Hoyle discovered that one theory about these objects does not apply in non-uniformly rotating examples. Eddington predicted the first observed gravitational redshift from an object of this kind, initially as a way to discredit Öpik's measurement of its density. These stars are supported by Fermi pressure. Found in the lower left of a standard Hertzsprung-Russell diagram, these stars are generally bounded in mass by a quantity equal to about 1.44 solar masses and known as the Chandrasekhar limit. For 10 points, name this class of stars, the endpoint for intermediate-mass main sequence stars, that are phenomenologically small stars that giving off incoherent light
Hoyle discovered that one theory about these objects does not apply in non-uniformly rotating examples.
{white dwarfs} [prompt on {population VII}]