Table 2.
Sample of cluster Cepheids found by our cross-match selection and in the literature.
| Cross-match |
Cluster parameters |
|||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Cepheid | Cluster | ϖ |  |
μδ | Age | Sep | Ref. | ϖCG18 | Nmemb | r50 | ⟨Vϖ⟩ | ϖadopted |
| (arcmin) | (mas) | (deg) | (μas2) | (mas) | ||||||||
| CV Mon | vdBergh 1 | • | • | • | • | 0.9 | a, b, c, d | 0.523±0.010 | 73 | 0.03 | 1741 | 0.523±0.043 |
| S Nor | NGC 6087 | • | • | • | • | 1.0 | a, b, c, e | 1.025±0.004 | 251 | 0.25 | 708 | 1.025±0.027 |
| U Sgr | IC 4725 | • | • | • | • | 2.1 | a, b, c | 1.514±0.003 | 516 | 0.26 | 563 | 1.514±0.024 |
| V367 Sct | NGC 6649 | • | • | • | • | 2.8 | a | 0.467±0.004 | 560 | 0.06 | 1689 | 0.467±0.041 |
| V Cen | NGC 5662 | • | • | • | • | 25 | a, b, c, f | 1.288±0.003 | 255 | 0.33 | 533 | 1.288±0.023 |
| RS Ori | FSR 0951 | • | • | • | 2.4 σ | 2.0 | PW | 0.553±0.004 | 195 | 0.16 | 697 | 0.553±0.027 |
| CS Vel | Ruprecht 79 | • | • | • | 2.5 σ | 2.2 | g | 0.221±0.004 | 178 | 0.05 | 1720 | 0.221±0.042 |
| DL Cas | NGC 129 | • | • | 3.4 σ | • | 3.4 | a, b, c | 0.511±0.002 | 392 | 0.17 | 904 | 0.511±0.031 |
| EV Sct | NGC 6664 | • | 1.1 σ | • | • | 2.4 | a | 0.468±0.004 | 237 | 0.10 | 1215 | 0.468±0.035 |
| V340 Nor | NGC 6067 | • | 1.3 σ | • | • | 0.9 | a, c | 0.443±0.002 | 995 | 0.11 | 1263 | 0.443±0.036 |
| CF Cas | NGC 7790 | • | 1.9 σ | • | • | 1.3 | a, b, c | 0.269±0.004 | 200 | 0.06 | 1642 | 0.269±0.041 |
| TW Nor | Lyngå 6 | • | 2.0 σ | • | 1.4 σ | 0.6 | a, b, c, h | 0.383±0.006 | 79 | 0.06 | 1730 | 0.383±0.042 |
| QZ Nor | NGC 6067 | • | 1.2 σ | 9 σ | • | 18 | a | 0.443±0.002 | 955 | 0.11 | 1263 | 0.443±0.036 |
| CG Cas | Berkeley 58 | • | 4.1 σ | 2.0 σ | 1.2 σ | 5.5 | a, b | 0.282±0.004 | 142 | 0.06 | 1661 | 0.282±0.041 |
Notes. Full circles stand for an agreement smaller than 1σ between the Cepheid and the cluster parameters.
References. (a): Anderson et al. (2013); (b): Chen et al. (2015); (c): An et al. (2007); (d): Turner et al. (1998); (e): Turner (1986); (f): Turner (1982); (g): Turner (2010); (h): Majaess et al. (2011; PW): present work.
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