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Table 3
Values of Teff and vsini used to create the atmospheric models and the synthetic profiles for the stars in Table 2.
| ID | Teff (K) | vsini (km s-1) | best fit model 4571 | best fit model b2 |
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|
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| HD 73722 | 6400 | 9 | m10_m60_100 | m10_m60_100 |
| IC 2391 73 | 6200 | 9 | m10_m60_100 | m10_m60_100 |
| HD 211415 | 5800 | 4 | m10_m60_100 | m10_m60_100 |
| HD 74497 | 5600 | 7 | m10_m60_075 | m10_m60_100 |
| IC 2391 98 | 5200 | 13 | m20_m60_100 | m10_m60_100 |
| HD 149661 | 5200 | 3 | m20_m60_075 | m10_m60_100 |
| HD 22049 | 5200 | 8 | m20_m60_075 | m10_m60_100 |
| HD 209100 | 4600 | 3 | m20_m60_075 | m10_m60_100 |
Notes. Indicated in the last two columns are the atmospheric models that best fit the observed profiles.
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