Collinder 139
(NGC 2374; MWSC 1206; OCL 585)
0.90
UTI
0.75
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
5.8 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Collinder 139 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 low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is very well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 111.014 | -13.246 | 0.767 | -4.638 | 0.687 | 46.334 |
| Li et al. | 2025 | 111.016 | -13.235 | 0.76 | -4.665 | 0.659 | â |
| Almeida et al. | 2025 | 111.0 | -13.236 | â | â | â | â |
| Hunt & Reffert | 2024 | 111.026 | -13.268 | 0.759 | -4.629 | 0.685 | 46.397 |
| Cavallo et al. | 2024 | 111.011 | -13.258 | 0.765 | â | â | â |
| Hunt & Reffert | 2023 | 111.026 | -13.268 | 0.759 | -4.629 | 0.685 | 46.397 |
| Almeida et al. | 2023 | 111.004 | -13.243 | â | â | â | â |
| Cordoni et al. | 2023 | 111.0 | -13.236 | 0.753 | -4.687 | 0.656 | â |
| Just et al. | 2023 | 110.994 | -13.267 | â | â | â | â |
| Tarricq et al. | 2022 | 111.031 | -13.236 | 0.765 | -4.628 | 0.695 | â |
| Jaehnig et al. | 2021 | 111.007 | -13.251 | 0.784 | -4.626 | 0.658 | â |
| Rain et al. | 2021 | 111.016 | -13.235 | 0.76 | -4.665 | 0.659 | â |
| Dias et al. | 2021 | 111.0 | -13.236 | 0.753 | -4.687 | 0.656 | â |
| Cantat-Gaudin et al. | 2020 | 111.016 | -13.235 | 0.76 | -4.665 | 0.659 | â |
| Cantat-Gaudin & Anders | 2020 | 111.016 | -13.235 | 0.76 | -4.665 | 0.659 | â |
| Bossini et al. | 2019 | 111.016 | -13.235 | â | â | â | â |
| Soubiran et al. | 2018 | 111.016 | -13.235 | â | â | â | 53.72 |
| Bica et al. | 2019 | 110.99 | -13.254 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 111.016 | -13.235 | 0.76 | -4.665 | 0.659 | â |
| Loktin & Popova | 2017 | 110.985 | -13.262 | â | -1.933 | -0.171 | 27.2 |
| Kharchenko et al. | 2016 | 110.994 | -13.267 | â | â | â | â |
| Dias et al. | 2014 | 110.983 | -13.263 | â | -1.78 | -0.76 | â |
| Kharchenko et al. | 2013 | 111.0 | -13.27 | â | -3.4 | -0.66 | 27.2 |
| Gozha et al. | 2012 | 110.983 | -13.263 | â | â | â | â |
| Piskunov et al. | 2008 | 110.981 | -13.259 | â | â | â | â |
| Kharchenko et al. | 2007 | 110.98 | -13.26 | â | 0.27 | â | â |
| Piskunov et al. | 2007 | 110.981 | -13.259 | â | â | â | â |
| van den Bergh | 2006 | 110.975 | -13.267 | â | â | â | â |
| Kharchenko et al. | 2005 | 110.98 | -13.26 | â | -3.85 | -1.14 | â |
| Kharchenko et al. | 2003 | 111.03 | -13.23 | â | -4.01 | -1.7 | â |
| Chen et al. | 2003 | 110.958 | -13.26 | â | -4.65 | -1.1 | 27.2 |
| Dias et al. | 2002 | 110.983 | -13.263 | â | -1.78 | -0.76 | 29.25 |
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 | 1.27 | 0.3 | 0.76 | 378 | 0.035 | 439 | 0.535 | 0.0 |
| Li et al. | 2025 | 1.20 | 0.42 | â | 416 | -0.030 | â | â | â |
| Almeida et al. | 2025 | 1.18 | 0.53 | â | 354 | â | 204 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 438(1) | â | â |
| Cavallo et al. | 2024 | 1.31 | 0.43 | â | 417 | 0.440 | â | â | â |
| Hunt & Reffert | 2023 | 1.22 | 0.30 | 0.76 | 455 | â | â | â | â |
| Almeida et al. | 2023 | 1.21 | 0.52 | â | 376 | 0.029 | 257(1) | 0.45 | â |
| Cordoni et al. | 2023 | 1.18 | 0.53 | â | 354 | 0.041 | 535 | 0.62 | 0.00 |
| Just et al. | 2023 | â | â | â | 562 | â | 244 | â | â |
| Tarricq et al. | 2022 | 1.18 | â | â | 309 | â | â | â | â |
| Jaehnig et al. | 2021 | 1.27(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 1.27 | 0.40 | â | 380 | â | â | â | 0 |
| Dias et al. | 2021 | 1.18 | 0.53 | â | 354 | 0.041 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.21 | 0.34 | â | 288 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.27 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 1.21 | 0.42 | â | 385 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 1.27 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.27 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.52 | 0.29 | â | 304 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.39 | 0.28 | â | 562 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.39 | 0.28 | â | 562 | â | â | â | â |
| Gozha et al. | 2012 | 1.47 | â | â | 290 | â | 1413 | â | â |
| Piskunov et al. | 2008 | 1.47 | 0.28 | â | 479 | â | 1445(1) | â | â |
| Piskunov et al. | 2007 | 1.47 | 0.28 | â | 479 | â | 440 | â | â |
| van den Bergh | 2006 | 1.47 | 0.28 | â | 288 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.47 | 0.28 | â | 479 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.49 | 0.28 | â | â | â | â | â | â |
| Chen et al. | 2003 | 1.47 | â | â | 290 | â | â | â | â |
| Dias et al. | 2002 | 1.47 | 0.28 | â | 290 | 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: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.