Selected properties of our He-core white dwarf sequences (metallicity of the progenitor star: Z = 0.03) at Teff ≈ 10 000 K.
|M∗/M⊙||MH/M∗ [10-3]||−log (1 − Mr/M∗)||τ [Myr = 106yr]|
Notes. The table lists the stellar mass, the mass of H in the outer envelope, the location of the He/H chemical interface, and the time it takes the star to cool from Teff ≈ 14 000 K to ≈8000 K.
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