Collinder 422
(NGC 6913; MWSC 3329; M 29; OCL 168)
0.95
UTI
0.76
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
11.5 [N/pc2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Collinder 422 is a rich, very dense object of very 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, very young cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a very small percentage of members with 3 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 | 99999â | 305.929 | 38.505 | 0.559 | -3.421 | -5.791 | -21.902 |
| Almeida et al. | 2025 | 305.912 | 38.484 | â | â | â | â |
| Hunt & Reffert | 2024 | 305.955 | 38.499 | 0.562 | -3.406 | -5.81 | -44.037 |
| Celli et al. | 2024 | 305.943 | 38.487 | â | â | â | â |
| Cavallo et al. | 2024 | 305.949 | 38.507 | 0.563 | â | â | â |
| Hunt & Reffert | 2023 | 305.955 | 38.499 | 0.562 | -3.406 | -5.81 | -44.037 |
| Almeida et al. | 2023 | 305.858 | 38.471 | â | â | â | â |
| Just et al. | 2023 | 305.995 | 38.507 | â | â | â | â |
| Jaehnig et al. | 2021 | 305.949 | 38.505 | 0.583 | -3.406 | -5.758 | â |
| Rain et al. | 2021 | 305.943 | 38.487 | 0.553 | -3.409 | -5.771 | â |
| Dias et al. | 2021 | 305.912 | 38.484 | 0.55 | -3.411 | -5.775 | â |
| Cantat-Gaudin et al. | 2020 | 305.943 | 38.487 | 0.553 | -3.409 | -5.771 | â |
| Cantat-Gaudin & Anders | 2020 | 305.943 | 38.487 | 0.553 | -3.409 | -5.771 | â |
| Bica et al. | 2019 | 305.987 | 38.502 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 305.943 | 38.487 | 0.553 | -3.409 | -5.771 | â |
| Loktin & Popova | 2017 | 305.985 | 38.508 | â | -1.703 | -0.861 | -19.6 |
| Kharchenko et al. | 2016 | 305.995 | 38.507 | â | â | â | â |
| Dias et al. | 2014 | 305.987 | 38.508 | â | -3.21 | -4.56 | â |
| Kharchenko et al. | 2013 | 306.0 | 38.51 | â | -4.0 | -5.2 | -19.6 |
| Gozha et al. | 2012 | 305.987 | 38.508 | â | â | â | â |
| Piskunov et al. | 2008 | 305.977 | 38.508 | â | â | â | â |
| Kharchenko et al. | 2007 | 305.98 | 38.51 | â | 0.11 | â | -21.05 |
| van den Bergh | 2006 | 305.983 | 38.523 | â | â | â | â |
| Kharchenko et al. | 2005 | 305.98 | 38.51 | â | -3.8 | -5.71 | -21.05 |
| Kharchenko et al. | 2003 | 306.0 | 38.5 | â | -3.23 | -5.36 | â |
| Chen et al. | 2003 | 305.977 | 38.508 | â | -2.95 | -6.16 | -34.0 |
| Dias et al. | 2002 | 305.988 | 38.508 | â | -3.21 | -4.56 | -16.9 |
| Dambis | 1999 | 305.983 | 38.523 | â | â | â | 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 | 1.53 | 2.785 | 2.43 | 13 | -0.121 | 571 | 0.6 | 0.0 |
| Almeida et al. | 2025 | 1.78 | 2.77 | â | 8 | â | 766 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 455(1) | â | â |
| Celli et al. | 2024 | â | â | â | 22 | â | 687 | â | â |
| Cavallo et al. | 2024 | 1.53 | 2.99 | â | 10 | -0.240 | â | â | â |
| Hunt & Reffert | 2023 | 1.74 | 2.86 | 2.43 | 6 | â | â | â | â |
| Almeida et al. | 2023 | 1.64 | 2.83 | â | 8 | -0.003 | 903(1) | 0.60 | â |
| Just et al. | 2023 | â | â | â | 32 | â | 43 | â | â |
| Jaehnig et al. | 2021 | 1.71(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 1.72 | 3.19 | â | 5 | â | â | â | 0 |
| Dias et al. | 2021 | 1.78 | 2.77 | â | 8 | 0.206 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.61 | 1.80 | â | 22 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.72 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.72 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.15 | 2.31 | â | 13 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.17 | 2.58 | â | 32 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.17 | 2.58 | â | 32 | â | â | â | â |
| Gozha et al. | 2012 | 1.15 | â | â | 13 | -0.550 | 27 | â | â |
| Piskunov et al. | 2008 | 1.15 | 3.04 | â | 13 | â | â | â | â |
| van den Bergh | 2006 | 1.15 | 2.29 | â | 13 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.15 | 3.04 | â | 13 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.15 | 2.29 | â | â | â | â | â | â |
| Chen et al. | 2003 | 1.15 | â | â | 10 | â | â | â | â |
| Dias et al. | 2002 | 1.54 | 3.19 | â | 5 | â | â | â | â |
| Dambis | 1999 | 1.15 | 2.80 | â | 10 | 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: good fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.