CWNU 1044
0.70
UTI
0.86
CN
1.0
Cdens
1.0
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
63.3 [arcmin]
- CN 0.86 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 1044 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
Note: This object shares a significant percentage of members with 3 later reported entries. See table with shared members information.
Very close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 128.872 | -51.186 | 2.819 | -12.556 | 9.896 | 19.045 |
| Wei et al. | 2025 | 128.802 | -50.971 | 2.893 | -12.789 | 9.989 | â |
| Hunt & Reffert | 2024 | 129.93 | -51.859 | 2.706 | -11.64 | 9.761 | 20.772 |
| Cavallo et al. | 2024 | 127.874 | -50.244 | 2.722 | â | â | â |
| Hunt & Reffert | 2023 | 129.93 | -51.859 | 2.706 | -11.64 | 9.761 | 20.772 |
| He et al. | 2022 | 128.236 | -50.693 | 2.818 | -12.441 | 9.907 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Wei et al. | 2025 | 0.37 | 0.62 | â | 10 | 0.500 | 217 | 0.54 | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 56* | â | â |
| Cavallo et al. | 2024 | 0.38 | 0.54 | â | 16 | -0.080 | â | â | â |
| Hunt & Reffert | 2023 | 0.36 | 0.15 | 0.91 | 34 | â | â | â | â |
| He et al. | 2022 | â | 0.40 | â | 40 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.