CWNU 1719
0.57
UTI
0.35
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
18.3 [N/pc2]
- CN 0.35 Poorly populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
CWNU 1719 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 269.954 | -21.56 | 0.316 | -0.39 | -2.008 | 94.422 |
| Hunt & Reffert | 2024 | 269.958 | -21.558 | 0.312 | -0.394 | -1.991 | 40.696 |
| Cavallo et al. | 2024 | 269.957 | -21.556 | 0.314 | â | â | â |
| Hunt & Reffert | 2023 | 269.958 | -21.558 | 0.312 | -0.394 | -1.991 | 40.696 |
| He et al. | 2023 | 269.956 | -21.554 | 0.324 | -0.424 | -2.004 | -13.05 |
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 | 2.78 | 4.93 | 2.29 | 11 | -0.240 | 1278 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1278(1) | â | â |
| Cavallo et al. | 2024 | 2.39 | 4.93 | â | 11 | -0.240 | â | â | â |
| Hunt & Reffert | 2023 | 2.78 | 4.80 | 2.29 | 18 | â | â | â | â |
| He et al. | 2023 | 3.24 | 5.60 | â | 3 | 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.