Dolidze 16
(FSR 0778; MWSC 491)
0.86
UTI
0.54
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
5.4 [arcmin]
- CN 0.54 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Dolidze 16 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is very well-studied in the literature.
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 | 78.612 | 32.742 | 0.784 | -0.094 | -2.681 | -11.011 |
| Almeida et al. | 2025 | 78.664 | 32.691 | â | â | â | â |
| Zhang et al. | 2024 | 78.593 | 32.77 | â | â | â | â |
| Hunt & Reffert | 2024 | 78.593 | 32.77 | 0.795 | -0.108 | -2.696 | -14.039 |
| Celli et al. | 2024 | 78.623 | 32.707 | â | â | â | â |
| Cavallo et al. | 2024 | 78.642 | 32.714 | 0.794 | â | â | â |
| Hunt & Reffert | 2023 | 78.593 | 32.77 | 0.795 | -0.108 | -2.696 | -14.039 |
| Just et al. | 2023 | 78.641 | 32.66 | â | â | â | â |
| Dias et al. | 2021 | 78.664 | 32.691 | 0.764 | -0.039 | -2.595 | â |
| Cantat-Gaudin et al. | 2020 | 78.623 | 32.707 | 0.762 | -0.063 | -2.602 | â |
| Cantat-Gaudin & Anders | 2020 | 78.623 | 32.707 | 0.762 | -0.063 | -2.602 | â |
| Cantat-Gaudin et al. | 2018 | 78.623 | 32.707 | 0.762 | -0.063 | -2.602 | â |
| Loktin & Popova | 2017 | 78.645 | 32.66 | â | 0.88 | -0.898 | -8.4 |
| Kharchenko et al. | 2016 | 78.641 | 32.66 | â | â | â | â |
| Dias et al. | 2014 | 78.683 | 32.689 | â | 0.49 | -4.12 | -8.4 |
| Kharchenko et al. | 2013 | 78.649 | 32.66 | â | 2.72 | -3.02 | â |
| Kharchenko et al. | 2012 | 78.649 | 32.66 | â | 2.72 | -3.02 | â |
| Froebrich et al. | 2007 | 78.583 | 32.795 | â | â | â | â |
| Dias et al. | 2002 | 78.683 | 32.689 | â | 0.49 | -4.12 | -8.4 |
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 | 1.26 | 1.26 | â | 12 | â | 229 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.182* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 261* | â | â |
| Celli et al. | 2024 | â | â | â | 17 | â | 216 | â | â |
| Cavallo et al. | 2024 | 1.28 | 1.14 | â | 12 | -0.020 | â | â | â |
| Hunt & Reffert | 2023 | 1.20 | 1.20 | 2.16 | 24 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 40 | â | 18 | â | â |
| Dias et al. | 2021 | 1.26 | 1.26 | â | 12 | -0.092 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.33 | 0.86 | â | 17 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.26 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.26 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.88 | 2.75 | â | 1514 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.87 | 1.03 | â | 40 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.87 | 1.03 | â | 40 | â | â | â | â |
| Kharchenko et al. | 2012 | 0.87 | 1.03 | â | 40 | â | â | â | â |
| Dias et al. | 2002 | 0.87 | 1.03 | 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: intermediate fit.
Cavallo et al. (2024)
Silver sample.