DC 3
(MWSC 1226)
0.81
UTI
0.63
CN
1.0
Cdens
1.0
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
0.9 [arcmin]
- CN 0.63 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
DC 3 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very large* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~12.02 kpc) differs significantly from the median photometric distance (~7.36 kpc).
Very distant
Moderate extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 111.755 | -37.516 | 0.083 | -1.222 | 2.731 | 102.568 |
| Hu & Soubiran | 2025 | 111.783 | -37.507 | â | â | â | â |
| Almeida et al. | 2025 | 111.751 | -37.52 | â | â | â | â |
| Hunt & Reffert | 2024 | 111.756 | -37.518 | 0.109 | -1.216 | 2.752 | 95.206 |
| Cavallo et al. | 2024 | 111.783 | -37.507 | 0.111 | â | â | â |
| He et al. | 2023 | 111.755 | -37.515 | 0.083 | -1.221 | 2.715 | 102.57 |
| Hunt & Reffert | 2023 | 111.756 | -37.518 | 0.109 | -1.216 | 2.752 | 95.206 |
| Just et al. | 2023 | 111.746 | -37.523 | â | â | â | â |
| Dias et al. | 2021 | 111.751 | -37.52 | 0.081 | -1.214 | 2.645 | â |
| Bica et al. | 2019 | 111.749 | -37.524 | â | â | â | â |
| Kharchenko et al. | 2016 | 111.746 | -37.523 | â | â | â | â |
| Kharchenko et al. | 2013 | 111.75 | -37.525 | â | -1.61 | 4.99 | â |
| Dias et al. | 2002 | 111.75 | -37.521 | â | -1.61 | 4.99 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.340* | â | â | â |
| Almeida et al. | 2025 | 7.93 | 1.04 | â | 2979 | â | 1659 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 359* | â | â |
| Cavallo et al. | 2024 | 7.45 | 0.96 | â | 4365 | -0.340 | â | â | â |
| He et al. | 2023 | 8.71 | 0.80 | â | 2512 | â | â | â | â |
| Hunt & Reffert | 2023 | 7.26 | 0.70 | 1.79 | 1629 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1820 | â | 170 | â | â |
| Dias et al. | 2021 | 7.93 | 1.04 | â | 2979 | -0.146 | â | â | â |
| Kharchenko et al. | 2016 | 4.32 | 1.68 | â | 1820 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.32 | 1.68 | â | 1820 | â | â | â | â |
| Dias et al. | 2002 | 4.32 | 1.68 | â | 1820 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.