CWNU 1088
- CN 0.25 Poorly populated
- Cdens 0.52 Moderately dense
- CC3 0.75 High quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 1088 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a very close distance, below the mid-plane. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | – | 86.078 | -1.433 | 2.218 | 1.621 | -4.027 | 10.31 |
| Zhang et al. | 2024 | 85.906 | -1.593 | – | – | – | – |
| Hunt & Reffert | 2024 | 85.906 | -1.593 | 2.213 | 1.698 | -4.061 | 17.033 |
| Cavallo et al. | 2024 | 86.548 | -1.313 | 2.21 | – | – | – |
| Hunt & Reffert | 2023 | 85.906 | -1.593 | 2.213 | 1.698 | -4.061 | 17.033 |
| He et al. | 2022 | 86.076 | -1.326 | 2.217 | 1.596 | -4.034 | – |
💡 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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | – | – | – | – | -0.075* | – | – | – |
| Hunt & Reffert | 2024 | – | – | – | – | – | 72* | – | – |
| Cavallo et al. | 2024 | 0.61 | 2.97 | – | 8 | 0.150 | – | – | – |
| Hunt & Reffert | 2023 | 0.44 | 2.52 | 2.38 | 30 | – | – | – | – |
| He et al. | 2022 | – | 4.10 | – | 3 | – | – | – | – |
💡 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.
