CWNU 62
0.47
UTI
0.33
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
8.7 [N/pc2]
- CN 0.33 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
CWNU 62 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 256.715 | -41.555 | 0.641 | 1.202 | -2.022 | 5.83 |
| Hunt & Reffert | 2024 | 256.701 | -41.565 | 0.632 | 1.203 | -1.996 | -18.327 |
| Cavallo et al. | 2024 | 256.708 | -41.594 | 0.633 | â | â | â |
| Hunt & Reffert | 2023 | 256.701 | -41.565 | 0.632 | 1.203 | -1.996 | -18.327 |
| He et al. | 2022 | 256.7 | -41.589 | 0.62 | 1.23 | -2.02 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.5 | 3.24 | 2.42 | 68 | 0.137 | 390 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 390(1) | â | â |
| Cavallo et al. | 2024 | 1.45 | 2.79 | â | 389 | 0.510 | â | â | â |
| Hunt & Reffert | 2023 | 1.50 | 3.24 | 2.42 | 68 | â | â | â | â |
| He et al. | 2022 | 1.58 | 3.60 | â | 25 | -0.236 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Cavallo et al. (2024)
Gold sample.