XDOCC 10
0.21
UTI
0.0
CN
0.04
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
Nm (P>50%)
23
Core radius and density
4.6 [pc], 0.2 [pc-2]
- CN 0.0 Sparse
- Cdens 0.04 Very loose
- CC3 1.0 Very high quality
- Clit 0.0 Rarely 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
XDOCC 10 is a sparse, very loose object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is rarely studied in the literature.
Note: This object shares a significant percentage of members with 3 later reported entries. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 305.525 | 37.238 | 0.501 | -2.402 | -5.264 | 53.948 |
| Jaehnig et al. | 2021 | 305.421 | 37.292 | 0.508 | -2.387 | -5.234 | 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 | 1.92 | 3.97 | â | 366 | 0.400 | 655 | 0.29 | â |
| Piatti et al. | 2023 | â | â | â | 708 | 0.400 | 655 | 0.29 | â |
| Jaehnig et al. | 2021 | 1.92(1) | 3.97 | â | 23 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
