Carbon burning
= Carbon burning
{wiki}
Carbon burning fuses carbon nuclei at temperatures of order $10^9\,\mathrm K$. In intermediate-mass stars it can ignite off-centre under partial electron degeneracy and propagate inward as a burning flame.
= Carbon burning
{wiki}
Carbon burning fuses carbon nuclei at temperatures of order $10^9\,\mathrm K$. In intermediate-mass stars it can ignite off-centre under partial electron degeneracy and propagate inward as a burning flame.