Collinder 469
(MWSC 2865; OCL 35)
0.87
UTI
0.61
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
2.3 [arcmin]
- CN 0.61 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very 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 and mass parameters (see Parameters). It is very well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 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 |
| 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 |
| Loktin & Popova | 2017 | 274.14 | -18.313 | β | 3.218 | -1.02 | 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 |
| 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 |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 2.04 | 1.95 | β | 274 | β | 159 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 700* | 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 |
| 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 |
| 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 |
| Loktin & Popova | 2017 | 1.51 | 1.37 | β | 71 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.28 | 3.55 | β | 100 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.28 | 3.55 | β | 100 | β | β | β | β |
| van den Bergh | 2006 | 1.48 | 1.30 | β | 63 | β | β | β | β |
| Dias et al. | 2002 | 1.48 | 1.30 | β | 63 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.