... stars

Strictly, Bergeat et al. (2002b) define new spectroscopic types, so we assume, as they state, that early-R stars are their HC' type, N stars their CV type.

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... cores

The energy released in their algorithm usually disrupts the star, which we consider unrealistic.

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... range

After some low-resolution trial runs the primary mass range was reduced to $0.3\leq M/{M_{\odot}}\leq8$ with little change to our results.

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... plane

Again, we associate their type CV stars with N stars, and their HC' stars with early-R stars.

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