Dolidze 1
(MWSC 3268)
0.41
UTI
0.0
CN
0.27
Cdens
0.5
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
4.6 [arcmin]
- CN 0.0 Sparse
- Cdens 0.27 Loose
- CC3 0.5 Intermediate quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
Dolidze 1 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is moderately studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate 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 | 302.37 | 36.47 | 0.339 | -2.617 | -5.076 | â |
| Almeida et al. | 2025 | 302.406 | 36.505 | â | â | â | â |
| Hunt & Reffert | 2024 | 302.364 | 36.493 | 0.333 | -2.583 | -5.074 | 8.857 |
| Cavallo et al. | 2024 | 302.358 | 36.469 | 0.334 | â | â | â |
| Hunt & Reffert | 2023 | 302.364 | 36.493 | 0.333 | -2.583 | -5.074 | 8.857 |
| Just et al. | 2023 | 302.422 | 36.495 | â | â | â | â |
| Dias et al. | 2021 | 302.406 | 36.505 | 0.288 | -2.721 | -4.961 | â |
| Loktin & Popova | 2017 | 302.415 | 36.506 | â | -0.627 | -1.472 | 4.0 |
| Kharchenko et al. | 2016 | 302.422 | 36.495 | â | â | â | â |
| Dias et al. | 2014 | 302.408 | 36.506 | â | -1.27 | -5.65 | 4.0 |
| Kharchenko et al. | 2013 | 302.427 | 36.498 | â | -1.59 | 0.09 | 4.0 |
| Dias et al. | 2002 | 302.408 | 36.506 | â | -1.27 | -5.65 | 4.0 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 2.86 | 2.05 | â | 12 | â | 380 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 285* | â | â |
| Cavallo et al. | 2024 | 2.47 | 1.82 | â | 14 | 0.170 | â | â | â |
| Hunt & Reffert | 2023 | 2.64 | 1.79 | 0.87 | 31 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 40 | â | 102 | â | â |
| Dias et al. | 2021 | 2.86 | 2.05 | â | 12 | 0.054 | â | â | â |
| Loktin & Popova | 2017 | 3.16 | 1.02 | â | 85 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.45 | 1.94 | â | 40 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.45 | 1.94 | â | 40 | â | â | â | â |
| Dias et al. | 2002 | 1.45 | 1.94 | â | 40 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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