CWNU 296
0.56
UTI
0.55
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
5.0 [arcmin]
- CN 0.55 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 296 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.
Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 277.238 | -14.248 | 0.52 | -0.075 | -0.993 | 22.307 |
| Hunt & Reffert | 2024 | 277.248 | -14.235 | 0.535 | -0.048 | -1.0 | â |
| Cavallo et al. | 2024 | 277.237 | -14.269 | 0.533 | â | â | â |
| Hunt & Reffert | 2023 | 277.248 | -14.235 | 0.535 | -0.048 | -1.0 | â |
| He et al. | 2022 | 277.23 | -14.296 | 0.53 | -0.1 | -1.02 | â |
đĄ 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 | â | â | â | â | â | 219* | â | â |
| Cavallo et al. | 2024 | 1.63 | 2.72 | â | 7 | -0.630 | â | â | â |
| Hunt & Reffert | 2023 | 1.81 | 1.78 | 0.55 | 70 | â | â | â | â |
| He et al. | 2022 | 2.45 | 0.24 | â | 3 | 0.611 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.