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Table 7.
Properties of the variable candidates in NGC 6441.
| ID | IDClement | IDOGLE | α (J2000) | δ (J2000) | Distance (a) | Period | AKs | ⟨Ks⟩ | Z − Ks | Y − Ks | J − Ks | H − Ks | μα* | μδ | Member (b) | Type |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (OGLE-BLG-) | (h:m:s) | (d:m:s) | (arcmin) | (days) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | (mas yr−1) | (mas yr−1) | ||||
| C1 | V57 | RRLYR-03918 | 17:50:10.40 | −37:02:55.9 | 0.54 | 0.694358 | 0.299 | 15.228 | 0.949 | 0.614 | 0.56 | 0.114 | −3.486 | −9.286 | Yes | RRab |
| C2 | V59 | RRLYR-03904 | 17:50:08.95 | −37:03:32.2 | 0.94 | 0.702823 | 0.416 | 15.347 | 0.861 | 0.582 | 0.451 | 0.042 | −7.74 | −0.528 | Yes | RRab |
| C3 | V66 | RRLYR-03934 | 17:50:11.45 | −37:02:07.0 | 1.0 | 0.860932 | 0.174 | 14.989 | 1.046 | 0.703 | 0.461 | 0.12 | −2.915 | −7.391 | Yes | RRab |
| C4 | V61 | RRLYR-03980 | 17:50:14.69 | −37:04:02.6 | 1.03 | 0.750108 | 0.278 | 15.173 | 1.031 | 0.706 | 0.467 | 0.092 | −1.965 | −4.983 | Yes | RRab |
| C5 | V62 | RRLYR-03961 | 17:50:13.19 | −37:04:06.5 | 1.04 | 0.679969 | 0.294 | 15.167 | 0.727 | 0.51 | 0.577 | 0.12 | −2.832 | −3.402 | Yes | RRab |
| C6 | V40 | RRLYR-03920 | 17:50:10.51 | −37:04:00.5 | 1.07 | 0.648005 | 0.343 | 15.3 | 1.024 | 0.705 | 0.389 | 0.087 | −0.95 | −5.497 | Yes | RRab |
| C7 | V43 | RRLYR-04003 | 17:50:16.85 | −37:02:09.7 | 1.19 | 0.773081 | 0.248 | 15.086 | 1.019 | 0.697 | 0.51 | 0.088 | −1.63 | −7.458 | Yes | RRab |
| C8 | V150 | – | 17:50:07.04 | −37:03:15.9 | 1.21 | 1.068624 | 0.184 | 14.709 | 1.058 | 0.754 | 0.467 | 0.11 | −2.487 | −5.487 | Yes | RRab |
| C9 | – | – | 17:50:05.90 | −37:03:20.7 | 1.44 | 2.93268 | 0.201 | 14.648 | 1.396 | 1.021 | 0.704 | 0.169 | −2.486 | −6.663 | Yes | ? |
| C10 | V42 | RRLYR-03956 | 17:50:13.05 | −37:01:31.5 | 1.54 | 0.812634 | 0.239 | 15.078 | 1.143 | 0.804 | 0.618 | 0.233 | −2.412 | −5.718 | Yes | RRab |
Notes. This table is available in its entirety at the CDS. A portion is shown here for guidance regarding its form and content.
(b)
Cluster membership according to criteria explained in Sect. 5.3.
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