CWNU 2049
0.15
UTI
0.28
CN
0.15
Cdens
0.38
CC3
0.06
Clit
0.79
Cdup
Nm (P>50%)
28
Core radius and density
2.1 [pc], 0.8 [pc-2]
- CN 0.28 Poorly populated
- Cdens 0.15 Very loose
- CC3 0.38 Low quality
- Clit 0.06 Rarely studied
- Cdup 0.79 Very likely unique
Overview
CWNU 2049 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.79) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 61.975 | 53.078 | 0.306 | -0.344 | -0.455 | -48.271 |
| Hunt & Reffert | 2024 | 61.973 | 53.106 | 0.3 | -0.334 | -0.45 | -48.272 |
| Cavallo et al. | 2024 | 61.971 | 53.085 | 0.299 | â | â | â |
| Hunt & Reffert | 2023 | 61.973 | 53.106 | 0.3 | -0.334 | -0.45 | -48.272 |
| He et al. | 2023 | 61.964 | 53.107 | 0.308 | -0.341 | -0.452 | -48.27 |
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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 3.3 | 2.43 | 1.07 | 290 | 0.320 | 262 | â | â |
| Hunt & Reffert | 2024 | 3.50 | 2.43 | 1.07 | 190 | â | 262(1) | â | â |
| Cavallo et al. | 2024 | 3.10 | 2.33 | â | 389 | 0.320 | â | â | â |
| Hunt & Reffert | 2023 | 3.50 | 2.43 | 1.07 | 191 | â | â | â | â |
| He et al. | 2023 | 3.02 | 2.45 | â | 447 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.88 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.88 (50th percentile).