Dolidze 8
0.79
UTI
0.66
CN
1.0
Cdens
0.75
CC3
0.78
Clit
1.0
Cdup
Stellar density (N50/rad)
34.5 [N/pc2]
- CN 0.66 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.78 Well-studied
- Cdup 1.0 Unique
Overview
Dolidze 8 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 306.122 | 42.297 | 1.025 | -2.525 | -6.118 | -14.463 |
| Almeida et al. | 2025 | 306.117 | 42.299 | â | â | â | â |
| Zhang et al. | 2024 | 306.126 | 42.29 | â | â | â | â |
| Hunt & Reffert | 2024 | 306.126 | 42.29 | 1.02 | -2.54 | -6.207 | -3.119 |
| Celli et al. | 2024 | 306.129 | 42.3 | â | â | â | â |
| Cavallo et al. | 2024 | 306.045 | 42.236 | 1.019 | â | â | â |
| Hunt & Reffert | 2023 | 306.126 | 42.29 | 1.02 | -2.54 | -6.207 | -3.119 |
| He et al. | 2022 | 306.103 | 42.289 | 1.018 | -2.537 | -6.155 | â |
| Dias et al. | 2021 | 306.117 | 42.299 | 0.986 | -2.661 | -6.033 | -2.968 |
| Cantat-Gaudin et al. | 2020 | 306.129 | 42.3 | 0.993 | -2.633 | -5.91 | â |
| Cantat-Gaudin & Anders | 2020 | 306.129 | 42.3 | 0.993 | -2.633 | -5.91 | â |
| Soubiran et al. | 2018 | 306.129 | 42.3 | â | â | â | -4.07 |
| Cantat-Gaudin et al. | 2018 | 306.129 | 42.3 | 0.993 | -2.633 | -5.91 | â |
| Loktin & Popova | 2017 | 306.09 | 42.281 | â | -0.581 | -1.692 | â |
| Dias et al. | 2002 | 306.096 | 42.281 | â | -12.96 | -4.4 | 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 | 0.98 | 1.7 | 2.27 | 5 | -0.108 | 107 | â | â |
| Almeida et al. | 2025 | 0.94 | 0.96 | â | 5 | â | 107 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.108(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 167(1) | â | â |
| Celli et al. | 2024 | â | â | â | 16 | â | 78 | â | â |
| Cavallo et al. | 2024 | 1.26 | 1.90 | â | 4 | -0.380 | â | â | â |
| Hunt & Reffert | 2023 | 0.96 | 1.50 | 2.27 | 4 | â | â | â | â |
| He et al. | 2022 | â | 1.25 | â | 3 | â | â | â | â |
| Dias et al. | 2021 | 0.94 | 0.96 | â | 5 | 0.372 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.05 | 2.22 | â | 15 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.98 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 0.98 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.98 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.01 | 2.13 | â | 15 | â | â | â | â |
| Dias et al. | 2002 | 1.08 | 5.16 | â | 716 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Wood sample.