Open Access
Table C.1.
Comparison to parameters determined in Carini et al. (2020) of the ten stars in common between the studies.
this work | Carini et al. (2020) | ||||||||
---|---|---|---|---|---|---|---|---|---|
ID | Teff | log g | v sin i | Flag | ID | Teff | log g | v sin i | |
[K] | [dex] | [km s−1] | [K] | [dex] | [km s−1] | ||||
670 | ![]() |
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A4 | 17000±1000 | 2.9±0.1 | 100 | ||
643 | ![]() |
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A5 | 21400±3000 | 3.5±0.2 | 250 | ||
313 | ![]() |
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SB1 | A10 | 20500±1000 | 3.7±0.1 | 200 | |
289 | ![]() |
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A17 | 21700±1000 | 3.6±0.1 | 100 | ||
420 | ![]() |
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A21 | 21000±1000 | 3.6±0.2 | 150 | ||
522 | ![]() |
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A23 | 21600±2000 | 3.6±0.2 | 100 | ||
573 | ![]() |
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A24 | 21700±1500 | 3.9±0.3 | 150 | ||
134 | ![]() |
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A34 | 20500±1500 | 3.8±0.2 | 150 | ||
228 | ![]() |
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A40 | 17500±500 | 3.1±0.1 | 100 | ||
519 | ![]() |
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SB1 | A48 | 22000±1500 | 3.1±0.3 | 150 |
Notes. Here, we use the parameters given in table 4 of Carini et al. (2020) which are based on their analysis considering stellar rotation. The two SB1s detected in Paper II are indicated in the column Flag.
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