CWNU 360
0.53
UTI
0.4
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
5.1 [N/pc2]
- CN 0.4 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High 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 360 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age parameter (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 | 234.506 | -57.091 | 0.386 | -3.604 | -2.669 | 14.079 |
| Hunt & Reffert | 2024 | 234.538 | -57.094 | 0.391 | -3.563 | -2.676 | 15.57 |
| Cavallo et al. | 2024 | 234.517 | -57.088 | 0.386 | â | â | â |
| Hunt & Reffert | 2023 | 234.538 | -57.094 | 0.391 | -3.563 | -2.676 | 15.57 |
| He et al. | 2022 | 234.53 | -57.082 | 0.39 | -3.6 | -2.68 | 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 | 2.38 | 3.69 | 2.02 | 107 | 0.899 | 568 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 568(1) | â | â |
| Cavallo et al. | 2024 | 2.61 | 3.69 | â | 107 | 0.830 | â | â | â |
| Hunt & Reffert | 2023 | 2.38 | 4.38 | 2.02 | 70 | â | â | â | â |
| He et al. | 2022 | 2.09 | 3.48 | â | 501 | 0.968 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Cavallo et al. (2024)
Silver sample.