Collinder 104
(MWSC 930)
0.75
UTI
0.62
CN
1.0
Cdens
0.75
CC3
0.69
Clit
1.0
Cdup
Stellar density (N50/rad)
7.2 [N/pc2]
- CN 0.62 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.69 Moderately studied
- Cdup 1.0 Unique
Overview
Collinder 104 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a 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.
Note: This object shares a small percentage of members with at least one entry reported in the same catalogue. 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 | 99.187 | 4.79 | 0.614 | -1.418 | 0.602 | 36.18 |
| Almeida et al. | 2025 | 99.157 | 4.816 | â | â | â | â |
| Zhang et al. | 2024 | 99.187 | 4.71 | â | â | â | â |
| Hunt & Reffert | 2024 | 99.187 | 4.71 | 0.62 | -1.391 | 0.651 | 30.638 |
| Cavallo et al. | 2024 | 99.288 | 4.838 | 0.62 | â | â | â |
| Hunt & Reffert | 2023 | 99.187 | 4.71 | 0.62 | -1.391 | 0.651 | 30.638 |
| Just et al. | 2023 | 99.105 | 4.774 | â | â | â | â |
| Dias et al. | 2021 | 99.157 | 4.816 | 0.514 | -1.23 | 0.507 | â |
| Loktin & Popova | 2017 | 99.12 | 4.818 | â | -0.206 | -0.584 | 6.33 |
| Kharchenko et al. | 2016 | 99.105 | 4.774 | â | â | â | â |
| Dias et al. | 2014 | 99.125 | 4.817 | â | -0.03 | -1.03 | 6.33 |
| Kharchenko et al. | 2013 | 99.112 | 4.773 | â | -1.99 | -1.74 | â |
| Dias et al. | 2002 | 99.125 | 4.817 | â | -0.03 | -1.03 | 6.33 |
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 | 1.81 | 2.275 | 2.09 | 166 | -0.104 | 307 | â | â |
| Almeida et al. | 2025 | 1.60 | 2.10 | â | 16 | â | 378 | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.080(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 307(1) | â | â |
| Cavallo et al. | 2024 | 1.45 | 1.79 | â | 19 | -0.480 | â | â | â |
| Hunt & Reffert | 2023 | 1.51 | 1.35 | 2.09 | 14 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 316 | â | 83 | â | â |
| Dias et al. | 2021 | 1.60 | 2.10 | â | 16 | -0.104 | â | â | â |
| Loktin & Popova | 2017 | 2.42 | 2.45 | â | 166 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.02 | 2.58 | â | 316 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.02 | 2.58 | â | 316 | â | â | â | â |
| Dias et al. | 2002 | 2.02 | 2.58 | â | 316 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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