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Table 4.

Quantities derived from the observed values given in Table 3.

Source Δ D 3 σ C 18 O $ \Delta D_{3\sigma}^\mathrm{C{18}O} $( † ) Mgas( ‡ ) f 13 CO $ f^{^{13}\rm CO} $ Δt 17O/18O M init KL 16 $ M^{\mathrm{KL16}}_{\mathrm{init}} $ M init FRUITY $ M^{\mathrm{FRUITY}}_{\mathrm{init}} $ LPAGB dmax
[au] [M] [×10−5] [yr] [M yr−1] [M] [M] [103L] [kpc]
GLMP 950 9360 0.10 1.1 1085 8 × 10−5 1.7 (0.2) 1.8 1.8 6.9 4.2
GLMP 953 11400 0.17 0.9 1460 1.1 × 10−4 1.3 (0.2) 1.7 1.7 6.7 4.0
AFGL 5385 14280 0.24 1.1 ( * ) 1510 1.7 × 10−4 0.61 (0.10) 1.4 1.5 5.9 2.4
HD 187885 ( † ) 8000 0.35 0.55 ( * ) 620 5 × 10−4 0.59 (0.12) 1.15 < 1.3 ∼6.2 ∼2.5
Hen 3-1475 16240 0.42 1.5 770 4 × 10−4 1.29 (0.15) 1.7 1.7 6.7 4.5
M1-92 22360 0.35 2.0 1190 2.5 × 10−4 1.8 (0.2) 1.8 1.8 6.9 2.8

Notes. ( † )Using the larger value of Δθ3σC18O. ( ‡ )For an assumed excitation temperature of 10 K and C18O abundance relative to the number of hydrogen nuclei of 2.1 × 10−7 for HD 187885 and 8.5 × 10−7 for the other sources (see Sect. 5.2). ( * )These values might be underestimated because the corresponding 13CO J = 2 − 1 line seems to be affected by optical depth effects.

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