Collinder 123
(NGC 2311; MWSC 1035; OCL 553; FSR 1127; FoF 931)
0.90
UTI
0.76
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
30.9 [N/pc2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Collinder 123 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low 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 very well-studied in the literature.
Note: This object shares a small percentage of members with 2 later reported entries. 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 | 99999β | 104.448 | -4.608 | 0.446 | -1.312 | 0.996 | 32.108 |
| Almeida et al. | 2025 | 104.464 | -4.619 | β | β | β | β |
| Hunt & Reffert | 2024 | 104.447 | -4.613 | 0.445 | -1.293 | 1.024 | 32.111 |
| Cavallo et al. | 2024 | 104.454 | -4.612 | 0.448 | β | β | β |
| Hunt & Reffert | 2023 | 104.447 | -4.613 | 0.445 | -1.293 | 1.024 | 32.111 |
| Almeida et al. | 2023 | 104.475 | -4.624 | β | β | β | β |
| Just et al. | 2023 | 104.438 | -4.608 | β | β | β | β |
| Jaehnig et al. | 2021 | 104.504 | -4.628 | 0.474 | -1.573 | 0.821 | β |
| Rain et al. | 2021 | 104.455 | -4.616 | 0.462 | -1.343 | 0.93 | β |
| Dias et al. | 2021 | 104.464 | -4.619 | 0.468 | -1.348 | 0.938 | β |
| Cantat-Gaudin et al. | 2020 | 104.455 | -4.616 | 0.462 | -1.343 | 0.93 | β |
| SΓ‘nchez et al. | 2020 | 104.446 | -4.612 | β | -1.356 | 1.006 | β |
| Donor et al. | 2020 | 104.445 | -4.61 | β | -1.46 | 0.8 | 100.5 |
| Cantat-Gaudin & Anders | 2020 | 104.455 | -4.616 | 0.462 | -1.343 | 0.93 | β |
| Liu & Pang | 2019 | 104.487 | -4.655 | 0.464 | -1.391 | 0.862 | β |
| Bica et al. | 2019 | 104.445 | -4.602 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 104.455 | -4.616 | 0.462 | -1.343 | 0.93 | β |
| Loktin & Popova | 2017 | 104.445 | -4.611 | β | 0.348 | 0.172 | β |
| Kharchenko et al. | 2016 | 104.438 | -4.608 | β | β | β | β |
| Dias et al. | 2014 | 104.446 | -4.612 | β | -1.48 | 3.31 | β |
| Kharchenko et al. | 2013 | 104.445 | -4.61 | β | -0.85 | 2.89 | β |
| Piskunov et al. | 2008 | 104.436 | -4.607 | β | β | β | β |
| van den Bergh | 2006 | 104.45 | -4.617 | β | β | β | β |
| Kharchenko et al. | 2005 | 104.44 | -4.61 | β | -3.2 | 2.77 | β |
| Kharchenko et al. | 2003 | 104.46 | -4.56 | β | -3.82 | 3.29 | β |
| Dias et al. | 2002 | 104.446 | -4.612 | β | -1.48 | 3.31 | β |
π‘ 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 | 99999β | 2.04 | 0.97 | 0.89 | 398 | -0.045 | 427 | 0.47 | 0.0 |
| Almeida et al. | 2025 | 1.84 | 1.09 | β | 60 | β | 435 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 419(1) | β | β |
| Cavallo et al. | 2024 | 2.10 | 0.85 | β | 100 | 0.400 | β | β | β |
| Hunt & Reffert | 2023 | 2.03 | 0.84 | 0.89 | 97 | β | β | β | β |
| Almeida et al. | 2023 | 1.91 | 1.19 | β | 63 | -0.045 | 365(1) | 0.47 | β |
| Just et al. | 2023 | β | β | β | 653 | β | 933 | β | β |
| Jaehnig et al. | 2021 | 2.10(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 2.04 | 1.02 | β | 398 | β | β | β | 0 |
| Dias et al. | 2021 | 1.84 | 1.09 | β | 60 | -0.079 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.00 | 1.00 | β | 45 | β | β | β | β |
| Donor et al. | 2020 | β | β | β | β | -0.320 | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.04 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 8 | 0.500 | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.04 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 3.12 | 0.97 | β | 479 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.22 | 0.64 | β | 653 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.22 | 0.64 | β | 653 | β | β | β | β |
| Piskunov et al. | 2008 | 2.00 | 0.62 | β | 398 | β | β | β | β |
| van den Bergh | 2006 | 2.29 | 1.02 | β | 398 | β | β | β | β |
| Kharchenko et al. | 2005 | 2.00 | 0.62 | β | 398 | β | β | β | β |
| Kharchenko et al. | 2003 | 2.29 | 0.87 | β | β | β | β | β | β |
| Dias et al. | 2002 | 2.29 | 1.02 | β | 398 | β | β | β | β |
(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: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.