Observed 17O/18O ratios and their uncertainties.
|Source||17O/18O||Mi (Stancliffe et al. 2004)||Mi (Karakas & Lugaro 2016)||Mi (Cristallo et al. 2011)|
|GX Mon||0.77 ± 0.16|
|WX Psc||0.26 ± 0.06||0.8 ≤ Mi ≤ 1.0||x|
|W Aql||1.17 ± 0.22|
|χ Cyg||2.00 ± 0.52|
|CW Leo||1.16 ± 0.06|
|LL Peg||0.56 ± 0.06|
|LP And||1.26 ± 0.08|
|RW LMi||1.36 ± 0.19|
|V384 Per||2.04 ± 0.32|
Notes. The final three columns denote the initial-mass estimates calculated from these ratios through comparison with stellar-evolution models.
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