Table 4.
Stellar parameters as re-derived here in the abundance analysis for the Romaniello et al. (2008) archival sample.
| CEP | v | dTeff | log(g) | dlog(g) | vturb | dvturb | Phase |
|---|---|---|---|---|---|---|---|
| OGLE107 | 5390 | 42 | 0.80 | 0.07 | 2.80 | 0.06 | 0.860 |
| OGLE461 | 4890 | 109 | 0.70 | 0.08 | 4.00 | 0.51 | 0.682 |
| OGLE655 | 5590 | 86 | 0.50 | 0.11 | 3.20 | 0.11 | 0.144 |
| OGLE945 | 4960 | 40 | 0.00 | 0.09 | 3.60 | 0.12 | 0.605 |
| OGLE1100 | 6200 | 122 | 0.70 | 0.16 | 3.10 | 0.17 | 0.201 |
| OGLE1128 | 5370 | 65 | 0.80 | 0.09 | 3.70 | 0.19 | 0.861 |
| OGLE1290 | 4870 | 64 | 0.10 | 0.08 | 4.00 | 1.04 | 0.136 |
| OGLE1327 | 5660 | 122 | 0.70 | 0.09 | 3.20 | 0.16 | 0.037 |
| OGLE2337 | 5590 | 56 | 0.40 | 0.09 | 3.20 | 0.12 | 0.130 |
| OGLE2832 | 5060 | 164 | 0.80 | 0.10 | 4.00 | 0.63 | 0.710 |
| … | … | … | … | … | … | … |
Notes. This table is available in its entirety at the CDS. OGLE510/HV879 is common to both samples and is considered here only once, namely in Table 3.
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