CWNU 15
0.24
UTI
0.0
CN
0.11
Cdens
0.5
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad)
0.5 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.11 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.3 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 15 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 87.409 | 26.122 | 0.861 | -0.396 | -2.685 | 1.683 |
| Zhang et al. | 2024 | 87.526 | 26.137 | â | â | â | â |
| Hunt & Reffert | 2024 | 87.526 | 26.137 | 0.863 | -0.401 | -2.632 | 11.537 |
| Cavallo et al. | 2024 | 87.464 | 25.982 | 0.863 | â | â | â |
| Hunt & Reffert | 2023 | 87.526 | 26.137 | 0.863 | -0.401 | -2.632 | 11.537 |
| He et al. | 2022 | 87.48 | 26.166 | 0.88 | -0.39 | -2.7 | 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 | 1.09 | 0.98 | 0.75 | 96 | -0.049 | 60 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.049(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 60(1) | â | â |
| Cavallo et al. | 2024 | 1.14 | 0.98 | â | 132 | 0.400 | â | â | â |
| Hunt & Reffert | 2023 | 1.09 | 0.95 | 0.75 | 96 | â | â | â | â |
| He et al. | 2022 | 0.93 | 1.44 | â | 32 | -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.