Collinder 43
(NGC 1444; MWSC 308; OCL 394)
0.90
UTI
0.76
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
12.9 [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 43 is a rich, very dense object of 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 age and metallicity parameters (see Parameters). It is very well-studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 57.354 | 52.657 | 0.864 | -0.762 | -1.837 | -6.105 |
| Li et al. | 2025 | 57.361 | 52.658 | 0.832 | -0.746 | -1.829 | β |
| Almeida et al. | 2025 | 57.344 | 52.651 | β | β | β | β |
| Zhang et al. | 2024 | 57.358 | 52.655 | β | β | β | β |
| Hunt & Reffert | 2024 | 57.358 | 52.655 | 0.874 | -0.802 | -1.844 | -10.062 |
| Celli et al. | 2024 | 57.361 | 52.658 | β | β | β | β |
| Cavallo et al. | 2024 | 57.352 | 52.647 | 0.875 | β | β | β |
| Hunt & Reffert | 2023 | 57.358 | 52.655 | 0.874 | -0.802 | -1.844 | -10.062 |
| Just et al. | 2023 | 57.338 | 52.638 | β | β | β | β |
| He et al. | 2022 | 57.344 | 52.643 | 0.869 | -0.767 | -1.855 | β |
| Jaehnig et al. | 2021 | 57.352 | 52.659 | 0.875 | -0.77 | -1.852 | β |
| Rain et al. | 2021 | 57.361 | 52.658 | 0.832 | -0.746 | -1.829 | β |
| Dias et al. | 2021 | 57.344 | 52.651 | 0.834 | -0.816 | -1.838 | β |
| Cantat-Gaudin et al. | 2020 | 57.361 | 52.658 | 0.832 | -0.746 | -1.829 | β |
| SΓ‘nchez et al. | 2020 | 57.354 | 52.658 | β | -0.695 | -1.953 | β |
| Cantat-Gaudin & Anders | 2020 | 57.361 | 52.658 | 0.832 | -0.746 | -1.829 | β |
| Soubiran et al. | 2018 | 57.361 | 52.658 | β | β | β | -36.9 |
| Bica et al. | 2019 | 57.341 | 52.642 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 57.361 | 52.658 | 0.832 | -0.746 | -1.829 | β |
| Loktin & Popova | 2017 | 57.36 | 52.658 | β | -0.067 | -2.104 | 2.0 |
| Kharchenko et al. | 2016 | 57.338 | 52.638 | β | β | β | β |
| Dias et al. | 2014 | 57.354 | 52.658 | β | -2.51 | -3.61 | β |
| Kharchenko et al. | 2013 | 57.349 | 52.64 | β | -2.26 | -4.2 | 2.0 |
| Kharchenko et al. | 2012 | 57.349 | 52.64 | β | -2.26 | -4.2 | 2.0 |
| Kharchenko et al. | 2007 | 57.36 | 52.66 | β | 0.03 | β | β |
| van den Bergh | 2006 | 57.35 | 52.667 | β | β | β | β |
| Dias et al. | 2002 | 57.354 | 52.658 | β | 2.34 | -1.95 | 2.0 |
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 | 1.16 | 2.01 | 1.58 | 10 | 0.011 | 112 | β | 2.0 |
| Li et al. | 2025 | 0.99 | 2.09 | β | 11 | -0.074 | β | β | β |
| Almeida et al. | 2025 | 1.10 | 2.01 | β | 14 | β | 92 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.158(1) | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 397(1) | β | β |
| Celli et al. | 2024 | β | β | β | 10 | β | 132 | β | β |
| Cavallo et al. | 2024 | 1.17 | 1.83 | β | 9 | 0.300 | β | β | β |
| Hunt & Reffert | 2023 | 1.10 | 1.95 | 1.58 | 7 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 7 | β | 40 | β | β |
| He et al. | 2022 | β | 2.25 | β | 10 | β | β | β | β |
| Jaehnig et al. | 2021 | 1.13(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 1.16 | 2.20 | β | 91 | β | β | β | 2 |
| Dias et al. | 2021 | 1.10 | 2.01 | β | 14 | 0.096 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.17 | 1.80 | β | 10 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.16 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 1.16 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.16 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.22 | 2.18 | β | 84 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.30 | 1.86 | β | 7 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.30 | 1.86 | β | 7 | β | β | β | β |
| Kharchenko et al. | 2012 | 1.30 | 1.86 | β | 7 | β | β | β | β |
| van den Bergh | 2006 | 1.20 | 2.20 | β | 91 | β | β | β | β |
| Dias et al. | 2002 | 1.20 | 2.21 | β | 92 | 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: worst fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.