CWWDL 13311
0.06
UTI
0.75
CN
0.21
Cdens
0.75
CC3
0.0
Clit
0.17
Cdup
Nm (P>50%)
106
Core radius and density
2.4 [pc], 1.1 [pc-2]
- CN 0.75 Rich
- Cdens 0.21 Very loose
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 0.17 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
CWWDL 13311 is a rich, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.
â ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 153.17 | -60.899 | 0.491 | -6.356 | 3.114 | -11.967 |
| Chi et al. | 2023 | 153.153 | -60.923 | 0.498 | -6.335 | 3.165 | -10.043 |
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 | â | â | â | 31 | -0.180 | â | â | â |
| Chi et al. | 2023 | â | â | â | 31 | -0.180 | â | â | â |
