Dol Dzim 4
(Dolidze-Dzimselejsvili 4; MWSC 592)
0.19
UTI
0.0
CN
0.0
Cdens
0.25
CC3
0.35
Clit
1.0
Cdup
Nm (P>50%)
16
Core radius and density
3.6 [pc], 0.02 [pc-2]
- CN 0.0 Sparse
- Cdens 0.0 Very loose
- CC3 0.25 Low quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
Dol Dzim 4 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~5.71 kpc) differs significantly from the median photometric distance (~1.66 kpc).
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 | 83.944 | 25.98 | 0.175 | 0.096 | -0.352 | -0.913 |
| Just et al. | 2023 | 83.951 | 25.95 | â | â | â | â |
| Donor et al. | 2020 | 83.975 | 25.95 | â | 0.64 | 0.23 | 48.0 |
| Dias et al. | 2018 | â | â | â | 2.07 | -3.74 | â |
| Dib et al. | 2018 | 83.959 | 25.95 | â | â | â | â |
| Sampedro et al. | 2017 | 83.975 | 25.95 | â | -0.6 | 1.3 | â |
| Joshi et al. | 2016 | 83.959 | 25.95 | â | â | â | â |
| Kharchenko et al. | 2016 | 83.951 | 25.95 | â | â | â | â |
| Tadross | 2014 | 83.975 | 25.95 | â | â | â | â |
| Dias et al. | 2014 | 83.975 | 25.95 | â | -1.11 | 1.39 | â |
| Kharchenko et al. | 2013 | 83.959 | 25.95 | â | 0.18 | -4.94 | â |
| Dias et al. | 2002 | 83.975 | 25.95 | â | -1.11 | 1.39 | â |
| Lynga | 1987 | 83.973 | 25.953 | â | â | â | 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 | 1.66 | 3.94 | â | 285 | -0.470 | 207 | â | â |
| Just et al. | 2023 | â | â | â | 285 | â | 207 | â | â |
| Spina et al. | 2022 | â | â | â | â | -0.470 | â | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.470 | â | â | â |
| Dib et al. | 2018 | 1.66 | â | â | 285 | â | â | â | â |
| Joshi et al. | 2016 | 1.66 | 3.94 | â | 285 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.66 | 3.94 | â | 285 | â | â | â | â |
| Tadross | 2014 | 1.22 | 3.47 | â | 100 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.66 | 3.94 | â | 285 | â | â | â | â |
| Dias et al. | 2002 | 1.22 | 3.47 | â | 100 | â | â | â | â |
MOCA
