A giant star's main-sequence progenitor had the solar-system value
PHYSICS · Multi-part · Fermi University Physics · Astrophysics & Cosmology · Stellar structure, energy generation and evolution · Stellar structure, energy generation and evolution
Stars from the Inside, Ch Stellar evolution: from the Hayashi track to the iron core, and the ages of clusters
Problem
A giant star's main-sequence progenitor had the solar-system value 12C/13C=89. After first dredge-up has deepened its convective envelope into layers once processed by the CN cycle in its hydrogen-burning core on the main sequence, spectroscopy of its surface gives 12C/13C=11.
((a)) State the range of 12C/13C that standard first dredge-up predicts for a low-mass giant, and say whether the observed value of 11 lies inside, above, or below it.
((b)) Predict what must additionally be happening in this giant if standard dredge-up alone cannot account for the observation, and state whether the responsible process is fully understood.