CWNU 1
0.00
UTI
0.32
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.0
Cdup
Stellar density (N50/rad)
15.1 [N/pc2]
- CN 0.32 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 0.0 Very likely duplicate
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 1 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near 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 parameter (see Parameters). It is rarely studied in the literature.
â ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 259.266 | -41.693 | 0.6 | -0.04 | -3.595 | -30.225 |
| Li et al. | 2023 | 259.264 | -41.687 | 0.59 | -0.05 | -3.58 | â |
| He et al. | 2022 | 259.257 | -41.692 | 0.6 | -0.03 | -3.58 | -18.1 |
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 | 1.805 | 2.75 | â | 730 | -0.583 | â | â | 1 |
| Li et al. | 2023 | 2.29 | 2.20 | â | 1259 | -0.524 | â | â | 1(1) |
| He et al. | 2022 | 1.32 | 3.30 | â | 200 | -0.642 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
