CWNU 367
0.26
UTI
0.0
CN
0.31
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
1.6 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.31 Loose
- 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 367 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, intermediate-age 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 | 274.124 | -12.687 | 0.669 | -1.137 | -0.594 | â |
| Hunt & Reffert | 2024 | 274.118 | -12.718 | 0.708 | -1.185 | -0.636 | 18.823 |
| Cavallo et al. | 2024 | 274.123 | -12.698 | 0.705 | â | â | â |
| Hunt & Reffert | 2023 | 274.118 | -12.718 | 0.708 | -1.185 | -0.636 | 18.823 |
| He et al. | 2022 | 274.111 | -12.72 | 0.69 | -1.06 | -0.58 | 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 | 1.36 | 1.57 | 1.69 | 407 | -0.944 | 127 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 127(1) | â | â |
| Cavallo et al. | 2024 | 1.36 | 1.57 | â | 407 | 0.140 | â | â | â |
| Hunt & Reffert | 2023 | 1.37 | 1.50 | 1.69 | 330 | â | â | â | â |
| He et al. | 2022 | 1.15 | 1.98 | â | 1259 | -2.028 | 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.