Collinder 469
(MWSC 2865; OCL 35)
0.82
UTI
0.61
CN
1.0
Cdens
0.75
CC3
0.87
Clit
1.0
Cdup
Nm (P>50%)
72
Core radius and density
0.8 [pc], 9.9 [pc-2]
- CN 0.61 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.87 Well-studied
- Cdup 1.0 Unique
Overview
Collinder 469 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 274.139 | -18.305 | 0.407 | 0.085 | -1.682 | 17.371 |
| Almeida et al. | 2025 | 274.138 | -18.318 | β | β | β | β |
| Hunt & Reffert | 2024 | 274.142 | -18.307 | 0.397 | 0.082 | -1.694 | β |
| Celli et al. | 2024 | 274.143 | -18.309 | β | β | β | β |
| Cavallo et al. | 2024 | 274.139 | -18.321 | 0.399 | β | β | β |
| Hunt & Reffert | 2023 | 274.142 | -18.307 | 0.397 | 0.082 | -1.694 | β |
| Just et al. | 2023 | 274.119 | -18.302 | β | β | β | β |
| Richer et al. | 2021 | 274.14 | -18.315 | 0.39 | 0.08 | -1.657 | β |
| Dias et al. | 2021 | 274.138 | -18.318 | 0.387 | 0.08 | -1.677 | β |
| Cantat-Gaudin et al. | 2020 | 274.143 | -18.309 | 0.399 | 0.089 | -1.679 | β |
| SΓ‘nchez et al. | 2020 | 274.142 | -18.312 | β | -0.061 | -1.453 | β |
| Cantat-Gaudin & Anders | 2020 | 274.143 | -18.309 | 0.399 | 0.089 | -1.679 | β |
| Soubiran et al. | 2018 | 274.143 | -18.309 | β | β | β | 17.84 |
| Bica et al. | 2019 | 274.139 | -18.314 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 274.143 | -18.309 | 0.399 | 0.089 | -1.679 | β |
| Dias et al. | 2018 | β | β | β | -0.57 | -1.54 | β |
| Dib et al. | 2018 | 274.126 | -18.3 | β | β | β | β |
| Loktin & Popova | 2017 | 274.14 | -18.313 | β | 3.218 | -1.02 | β |
| Sampedro et al. | 2017 | 274.142 | -18.312 | β | 0.57 | 0.16 | β |
| Joshi et al. | 2016 | 274.126 | -18.3 | β | β | β | β |
| Kharchenko et al. | 2016 | 274.119 | -18.302 | β | β | β | β |
| Dias et al. | 2014 | 274.142 | -18.312 | β | 1.09 | -1.52 | β |
| Kharchenko et al. | 2013 | 274.126 | -18.3 | β | 1.78 | -2.03 | β |
| Morales et al. | 2013 | 274.142 | -18.312 | β | β | β | β |
| Bukowiecki et al. | 2011 | 274.142 | -18.302 | β | β | β | β |
| van den Bergh | 2006 | 274.1 | -18.217 | β | β | β | β |
| Dias et al. | 2002 | 274.142 | -18.312 | β | 1.09 | -1.52 | β |
| Lynga | 1987 | 274.109 | -18.219 | β | β | β | 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 | 1.99 | 2.07 | 2.5 | 71 | -0.150 | 380 | β | β |
| Almeida et al. | 2025 | 2.04 | 1.95 | β | 274 | β | 159 | β | β |
| Hunt & Reffert | 2024 | 2.27 | 2.07 | 2.50 | 35 | β | 700(1) | β | β |
| Celli et al. | 2024 | β | β | β | 10 | β | 380 | β | β |
| Cavallo et al. | 2024 | 2.01 | 2.89 | β | 23 | -0.570 | β | β | β |
| Hunt & Reffert | 2023 | 2.27 | 2.07 | 2.50 | 35 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 100 | β | 90 | β | β |
| Richer et al. | 2021 | β | 2.40 | β | β | β | β | β | β |
| Dias et al. | 2021 | 2.04 | 1.95 | β | 274 | 0.270 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.42 | 1.96 | β | 10 | β | β | β | β |
| Kounkel et al. | 2020 | 2.36 | 2.31 | β | 138 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.34 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 2.34 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.34 | β | β | β | β | β | β | β |
| Dib et al. | 2018 | 1.28 | β | β | 100 | β | β | β | β |
| Loktin & Popova | 2017 | 1.51 | 1.39 | β | 71 | β | β | β | β |
| Joshi et al. | 2016 | 1.28 | 3.61 | β | 100 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.28 | 3.61 | β | 100 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.28 | 3.61 | β | 100 | β | β | β | β |
| Morales et al. | 2013 | 1.48 | β | β | 63 | β | β | β | β |
| Bukowiecki et al. | 2012 | β | β | β | β | β | 1028 | β | β |
| Bukowiecki et al. | 2011 | 1.48(1) | 2.05 | β | 112 | β | β | β | β |
| van den Bergh | 2006 | 1.48 | 1.32 | β | 63 | β | β | β | β |
| Dias et al. | 2002 | 1.48 | 1.32 | β | 63 | β | β | β | β |
| Lynga | 1987 | 1.97 | 2.27 | β | 20 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P284, along with HSC_161.
Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.22 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.22 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1353, e_all=0.0111.
Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.