A new synthetic model for asymptotic giant branch stars
We present a synthetic model for thermally pulsing asymptotic giant branch (TPAGB) evolution constructed by fitting expressions to full evolutionary models in the metallicity range 0.0001 ≤ Z ≤ 0.02. Our model includes parametrizations of third dredge
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
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