XDOCC 02
0.59
UTI
0.51
CN
0.92
Cdens
0.75
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members)
8.7 [arcmin]
- CN 0.51 Moderately populated
- Cdens 0.92 Very dense
- CC3 0.75 High quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
XDOCC 02 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above 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.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Relatively close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 84.063 | 34.298 | 0.753 | 0.268 | -2.359 | 9.721 |
| Zhang et al. | 2024 | 84.033 | 34.291 | â | â | â | â |
| Hunt & Reffert | 2024 | 84.033 | 34.291 | 0.756 | 0.264 | -2.356 | 4.086 |
| Cavallo et al. | 2024 | 84.065 | 34.298 | 0.755 | â | â | â |
| Hunt & Reffert | 2023 | 84.033 | 34.291 | 0.756 | 0.264 | -2.356 | 4.086 |
| Jaehnig et al. | 2021 | 84.049 | 34.298 | 0.801 | 0.285 | -2.295 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.344* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 191* | â | â |
| Cavallo et al. | 2024 | 1.28 | 0.85 | â | 56 | -0.390 | â | â | â |
| Hunt & Reffert | 2023 | 1.25 | 0.51 | 0.43 | 35 | â | â | â | â |
| Piatti et al. | 2023 | â | â | â | 30 | 0.240 | 343 | 0.45 | â |
| Jaehnig et al. | 2021 | 1.26* | 0.57 | â | 35 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.