- ... 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
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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