Table 6
CNO affects on the mass-loss rates of all the sample.
| Star | Ṁderived (a) (M⊙ yr−1) |  (M⊙ yr−1) |
C/H, N/H, O/H (× 10−4) | ||
|---|---|---|---|---|---|
| HD 156292 |  |
 |
* 0.7, 1.6, 1.1 | ||
| HD 24431 |  |
 |
1.3, 0.8, 3.9 | ||
| HD 105627 |  |
 |
* 0.7, 1.6, 1.1 | ||
| HD 116852 |  |
✓ | * 0.7, 1.6, 1.1 | ||
| HD 153426 |  |
✓ | 2.9, 1.0, 4.6 | ||
| HD 218195 |  |
✓ | 2.0, 5.0, 4.6 | ||
| HD 36861 |  |
✓ | 2.2, 1.5, 4.7 | ||
| HD 115455 |  |
 |
* 0.7, 1.6, 1.1 | ||
| HD 135591 |  |
✓ | * 0.7, 1.6, 1.1 |
Notes. Revised mass-loss rates are denoted by 
. The tick symbol (✓) stands for star without changes in Ṁ. In the last column, the asterisk symbol (*) stands for adopted ɛCNO. The Ṁderived were determined using solar ɛCNO from Grevesse et al. (2010): C/H = 2.7 × 10−4, N/H = 0.7 × 10−4, and O/H = 4.9 × 10−4. (a) Same notation as in Table 3.
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