CWNU 1755
0.23
UTI
0.35
CN
0.18
Cdens
0.25
CC3
0.19
Clit
1.0
Cdup
Nm (P>50%)
35
Core radius and density
2.3 [pc], 0.9 [pc-2]
- CN 0.35 Poorly populated
- Cdens 0.18 Very loose
- CC3 0.25 Low quality
- Clit 0.19 Rarely studied
- Cdup 1.0 Unique
Overview
CWNU 1755 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) 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 | 97.571 | 10.004 | 0.289 | 0.858 | -1.438 | 37.906 |
| Zhang et al. | 2024 | 97.579 | 10.01 | â | â | â | â |
| Hunt & Reffert | 2024 | 97.579 | 10.01 | 0.287 | 0.861 | -1.438 | 49.923 |
| Cavallo et al. | 2024 | 97.548 | 10.021 | 0.284 | â | â | â |
| Hunt & Reffert | 2023 | 97.579 | 10.01 | 0.287 | 0.861 | -1.438 | 49.923 |
| He et al. | 2023 | 97.577 | 9.997 | 0.306 | 0.872 | -1.456 | 37.91 |
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 | 3.04 | 2.84 | 2.75 | 820 | -0.146 | 522 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.512(1) | â | â | â |
| Hunt & Reffert | 2024 | 2.92 | 2.59 | 2.75 | 846 | â | 522(1) | â | â |
| Cavallo et al. | 2024 | 4.83 | 3.09 | â | 339 | 0.220 | â | â | â |
| Hunt & Reffert | 2023 | 2.92 | 2.59 | 2.75 | 847 | â | â | â | â |
| He et al. | 2023 | 3.16 | 3.25 | â | 794 | 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)
Silver sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 0.01 (50th percentile), false positive (human-assigned).
Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 0.01 (50th percentile), false positive (human-assigned).