Collinder 432
(IC 1369; MWSC 3481; OCL 204; FSR 0285; FoF 342)
0.93
UTI
0.88
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
3.5 [arcmin]
- CN 0.88 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Collinder 432 is a rich, 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 massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is very well-studied in the literature.
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
Distant
Moderate extinction
Massive
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 318.033 | 47.773 | 0.273 | -4.612 | -5.622 | -49.105 |
| Li et al. | 2025 | 318.033 | 47.77 | 0.262 | -4.644 | -5.609 | β |
| Almeida et al. | 2025 | 318.024 | 47.768 | β | β | β | β |
| Hunt & Reffert | 2024 | 318.033 | 47.776 | 0.271 | -4.603 | -5.629 | -45.727 |
| Cavallo et al. | 2024 | 318.041 | 47.781 | 0.264 | β | β | β |
| Hunt & Reffert | 2023 | 318.033 | 47.776 | 0.271 | -4.603 | -5.629 | -45.727 |
| Almeida et al. | 2023 | 318.019 | 47.77 | β | β | β | β |
| Just et al. | 2023 | 318.043 | 47.752 | β | β | β | β |
| Jaehnig et al. | 2021 | 318.029 | 47.769 | 0.288 | -4.641 | -5.6 | β |
| Rain et al. | 2021 | 318.033 | 47.77 | 0.262 | -4.644 | -5.609 | β |
| Dias et al. | 2021 | 318.024 | 47.768 | 0.265 | -4.638 | -5.6 | -47.338 |
| Cantat-Gaudin et al. | 2020 | 318.033 | 47.77 | 0.262 | -4.644 | -5.609 | β |
| SΓ‘nchez et al. | 2020 | 318.025 | 47.733 | β | -4.618 | -5.631 | β |
| Donor et al. | 2020 | 318.048 | 47.755 | β | -4.68 | -5.55 | -48.5 |
| Cantat-Gaudin & Anders | 2020 | 318.033 | 47.77 | 0.262 | -4.644 | -5.609 | β |
| Liu & Pang | 2019 | 318.03 | 47.772 | 0.28 | -4.652 | -5.604 | β |
| Bossini et al. | 2019 | 318.033 | 47.77 | β | β | β | β |
| Soubiran et al. | 2018 | 318.033 | 47.77 | β | β | β | -48.25 |
| Bica et al. | 2019 | 318.029 | 47.764 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 318.033 | 47.77 | 0.262 | -4.644 | -5.609 | β |
| Loktin & Popova | 2017 | 318.03 | 47.755 | β | -0.869 | -0.083 | β |
| Kharchenko et al. | 2016 | 318.043 | 47.752 | β | β | β | β |
| Dias et al. | 2014 | 318.025 | 47.733 | β | -3.36 | -5.37 | β |
| Kharchenko et al. | 2013 | 318.048 | 47.755 | β | -4.02 | -0.91 | β |
| van den Bergh | 2006 | 318.025 | 47.733 | β | β | β | β |
| Dias et al. | 2002 | 318.025 | 47.733 | β | -3.36 | -5.37 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 2.83 | 2.63 | β | 342 | -0.021 | β | β | β |
| Almeida et al. | 2025 | 2.81 | 2.49 | β | 331 | β | 1374 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 3589* | β | β |
| Cavallo et al. | 2024 | 3.28 | 2.84 | β | 219 | 0.170 | β | β | β |
| Hunt & Reffert | 2023 | 3.42 | 2.79 | 1.70 | 184 | β | β | β | β |
| Almeida et al. | 2023 | 2.87 | 2.56 | β | 309 | -0.009 | 1262* | 0.67 | β |
| Just et al. | 2023 | β | β | β | 347 | β | 731 | β | β |
| Jaehnig et al. | 2021 | 3.48* | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 3.44 | 2.05 | β | 288 | β | β | β | 0 |
| Dias et al. | 2021 | 2.81 | 2.49 | β | 331 | -0.023 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 3.30 | 2.11 | β | 288 | β | β | β | β |
| Donor et al. | 2020 | β | β | β | β | -0.080 | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.44 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 741 | 0.500 | β | β | β |
| Bossini et al. | 2019 | 3.23 | 2.05 | β | 290 | 0.090 | β | β | β |
| Soubiran et al. | 2018 | 3.44 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.44 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 2.27 | 1.75 | β | 457 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.53 | 1.78 | β | 347 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.53 | 1.78 | β | 347 | β | β | β | β |
| van den Bergh | 2006 | 2.08 | 1.77 | β | 437 | β | β | β | β |
| Dias et al. | 2002 | 2.08 | 1.77 | β | 437 | 0.090 | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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