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Table 5

Comparison of our adopted broadening parameters with those obtained via IACOB-BROAD (Simón-Díaz & Herrero 2014) applied to high-resolution MIKE data.

Star By eye+XShootU IACOB-BROAD+MIKE
vrot sin i km s-1 vmac km s-1 vrot sin i km S-1 vmac km s-1 line
AzV 327 55 20 6462+35Mathematical equation: $64_{ - 62}^{ + 35}$ 8755+42Mathematical equation: $87_{ - 55}^{ + 42}$ Si iii λ4552
AzV 104 65 20 8053+19Mathematical equation: $80_{ - 53}^{ + 19}$ 4543+63Mathematical equation: $45_{ - 43}^{ + 63}$ Si iii λ4552
AzV 96 50 20 5224+16Mathematical equation: $52_{ - 24}^{ + 16}$ 5929+23Mathematical equation: $59_{ - 29}^{ + 23}$ Si iii λ4552
AzV 264 45 20 4543+15Mathematical equation: $45_{ - 43}^{ + 15}$ 3331+39Mathematical equation: $33_{ - 31}^{ + 39}$ Si iii λ4552
AzV 18 50 20 4318+11Mathematical equation: $43_{ - 18}^{ + 11}$ 4421+20Mathematical equation: $44_{ - 21}^{ + 20}$ Si iii λ4552
NGC330-ELS-4 35 20 3318+9Mathematical equation: $33_{ - 18}^{ + 9}$ 2919+19Mathematical equation: $29_{ - 19}^{ + 19}$ Si iii λ4552
AzV 187 40 20 3634+17Mathematical equation: $36_{ - 34}^{ + 17}$ 4135+27Mathematical equation: $41_{ - 35}^{ + 27}$ Si iii λ4552
AzV 393 30 20 3532+16Mathematical equation: $35_{ - 32}^{ + 16}$ 3028+33Mathematical equation: $30_{ - 28}^{ + 33}$ Si iii λ4552
AzV 343 35 20 4421+9Mathematical equation: $44_{ - 21}^{ + 9}$ 1917+33Mathematical equation: $19_{ - 17}^{ + 33}$ Si ii λ6347
AzV 324 25 20 219+6Mathematical equation: $21_{ - 9}^{ + 6}$ 2610+8Mathematical equation: $26_{ - 10}^{ + 8}$ Si ii λ6347

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