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Table 2.

Definitions of stellar subtypes in populations.

Subtype Definition
MS Xc ≥ 10−5(†)
Post-MS Xc < 10−5
SG Post-MS and log(L [L]) > 4 and Xs > 0.35 (†)
BSG SG and log(Teff [K]) ≥ 3.9
YSG SG and 3.66 < log(Teff [K]) < 3.9
RSG SG and log(Teff[K]) ≤ 3.66
WR log(Teff[K]) > 4 and Xs ≤ 0.35
WNL WR and Xs ≥ 10−5
WNE WR and Xs < 10−5 and Cs ≤ Ns(†)
WNC WR and Xs < 10−5 and 0.1 ≤ Cs/Ns ≤ 10
WC WR and Xs < 10−5 and Cs + Os ≤ Ys(†) (numb. frac.)
WO WR and Xs < 10−5 and Cs + Os > Ys (numb. frac.)

Notes.

(†)

X, Y, C, N, and O refer to the mass fractions (unless ‘numb. frac.’ is specified, in which case they are the number fractions) of 1H, 4He, 12C, 14N, and 16O, respectively. The subscripts c (centre) and s (surface) refer to where in a star these abundances are taken.

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