Collinder 428
0.57
UTI
0.48
CN
0.64
Cdens
0.75
CC3
0.5
Clit
1.0
Cdup
Stellar density (N50/rad)
3.2 [N/pc2]
- CN 0.48 Poorly populated
- Cdens 0.64 Moderately dense
- CC3 0.75 High quality
- Clit 0.5 Moderately studied
- Cdup 1.0 Unique
Overview
Collinder 428 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a very large* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~10.25 kpc) differs significantly from the median photometric distance (~3.39 kpc).
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 315.741 | 44.503 | 0.098 | -2.911 | -3.039 | -86.071 |
| Hu & Soubiran | 2025 | 315.745 | 44.495 | â | â | â | â |
| Zhang et al. | 2024 | 315.742 | 44.5 | â | â | â | â |
| Hunt & Reffert | 2024 | 315.742 | 44.5 | 0.088 | -2.889 | -3.063 | -72.031 |
| Cavallo et al. | 2024 | 315.744 | 44.495 | 0.097 | â | â | â |
| Hunt & Reffert | 2023 | 315.742 | 44.5 | 0.088 | -2.889 | -3.063 | -72.031 |
| Loktin & Popova | 2017 | 315.795 | 44.583 | â | -1.213 | -0.257 | â |
| Dias et al. | 2014 | 315.8 | 44.583 | â | -3.13 | -1.47 | â |
| Kharchenko et al. | 2003 | 315.76 | 44.58 | â | -0.5 | -0.55 | â |
| Dias et al. | 2002 | 315.8 | 44.583 | â | -3.13 | -1.47 | 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 | 3.39 | 1.4 | 1.57 | 603 | 0.002 | 1156 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.230(5) | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.002(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1156(1) | â | â |
| Cavallo et al. | 2024 | 4.59 | 1.83 | â | 794 | 0.390 | â | â | â |
| Hunt & Reffert | 2023 | 7.68 | 2.90 | 1.57 | 158 | â | â | â | â |
| Loktin & Popova | 2017 | 3.39 | 1.40 | â | 603 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.00 | 0.31 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.00 | 0.31 | â | â | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.