CWNU 117
- CN 0.3 Poorly populated
- Cdens 0.42 Loose
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 0.17 Likely duplicate
Overview
CWNU 117 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature. Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | – | 341.242 | 57.525 | 0.639 | -3.949 | -2.97 | -24.995 |
| Hunt & Reffert | 2024 | 341.148 | 57.53 | 0.637 | -3.947 | -2.968 | -24.987 |
| Cavallo et al. | 2024 | 341.222 | 57.498 | 0.64 | – | – | – |
| Hunt & Reffert | 2023 | 341.148 | 57.53 | 0.637 | -3.947 | -2.968 | -24.987 |
| He et al. | 2022 | 341.204 | 57.538 | 0.64 | -3.95 | -2.97 | -26.3 |
💡 Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | – | – | – | – | – | 126* | – | – |
| Cavallo et al. | 2024 | 1.74 | 1.39 | – | 78 | 0.160 | – | – | – |
| Hunt & Reffert | 2023 | 1.52 | 0.94 | 0.38 | 155 | – | – | – | – |
| He et al. | 2022 | 1.48 | 1.38 | – | 126 | -0.642 | – | – | – |
💡 Note: The parameters are sometimes
transformed from their original values to match the format of the
columns shown here, see FAQ.
The columns DAv, Bfr, BSS correspond to differential
extinction, binary fraction, and blue stragglers, respectively.
BSS values can be listed as fractions or integers.
(*): indicates that this parameter is
assigned more than one value in the corresponding reference.
