Collinder 313
(VDBH 198; NGC 6208; MWSC 2470; OCL 964; vdBergh-Hagen 198; ESO 179 14; FSR 1724; FoF 2063)
0.97
UTI
0.84
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
44.5 [N/pc2]
- CN 0.84 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Collinder 313 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity and mass 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 | 99999â | 252.338 | -53.721 | 0.844 | -1.001 | -1.523 | -32.461 |
| Li et al. | 2025 | 252.336 | -53.714 | 0.83 | -0.966 | -1.519 | â |
| Hu & Soubiran | 2025 | 252.334 | -53.72 | â | â | â | â |
| Wei et al. | 2025 | 252.332 | -53.73 | 0.845 | -1.005 | -1.525 | â |
| Almeida et al. | 2025 | 252.327 | -53.713 | â | â | â | â |
| Hunt & Reffert | 2024 | 252.344 | -53.712 | 0.846 | -1.015 | -1.521 | -32.727 |
| Cavallo et al. | 2024 | 252.334 | -53.72 | 0.847 | â | â | â |
| Hunt & Reffert | 2023 | 252.344 | -53.712 | 0.846 | -1.015 | -1.521 | -32.727 |
| Almeida et al. | 2023 | 252.304 | -53.708 | â | â | â | â |
| Cordoni et al. | 2023 | 252.327 | -53.713 | 0.832 | -0.974 | -1.502 | â |
| Just et al. | 2023 | 252.333 | -53.715 | â | â | â | â |
| He et al. | 2022 | 252.335 | -53.727 | 0.849 | -1.006 | -1.528 | â |
| Tarricq et al. | 2022 | 252.351 | -53.717 | 0.838 | -0.994 | -1.527 | â |
| Dias et al. | 2021 | 252.327 | -53.713 | 0.832 | -0.974 | -1.502 | -31.761 |
| Cantat-Gaudin et al. | 2020 | 252.336 | -53.714 | 0.83 | -0.966 | -1.519 | â |
| Cantat-Gaudin & Anders | 2020 | 252.336 | -53.714 | 0.83 | -0.966 | -1.519 | â |
| Liu & Pang | 2019 | 252.343 | -53.725 | 0.842 | -0.952 | -1.506 | â |
| Bossini et al. | 2019 | 252.336 | -53.714 | â | â | â | â |
| Soubiran et al. | 2018 | 252.336 | -53.714 | â | â | â | -32.15 |
| Bica et al. | 2019 | 252.355 | -53.729 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 252.336 | -53.714 | 0.83 | -0.966 | -1.519 | â |
| Loktin & Popova | 2017 | 252.36 | -53.729 | â | 1.653 | 0.238 | -32.2 |
| Kharchenko et al. | 2016 | 252.333 | -53.715 | â | â | â | â |
| Dias et al. | 2014 | 252.367 | -53.728 | â | -1.97 | -5.01 | â |
| Kharchenko et al. | 2013 | 252.345 | -53.715 | â | -3.15 | -2.2 | -32.2 |
| Gozha et al. | 2012 | 252.367 | -53.728 | â | â | â | â |
| Piskunov et al. | 2008 | 252.356 | -53.729 | â | â | â | â |
| Kharchenko et al. | 2007 | 252.36 | -53.73 | â | 0.14 | â | â |
| van den Bergh | 2006 | 252.367 | -53.728 | â | â | â | â |
| Kharchenko et al. | 2005 | 252.36 | -53.73 | â | -0.91 | -4.72 | â |
| Chen et al. | 2003 | 252.355 | -53.729 | â | â | â | â |
| Dias et al. | 2002 | 252.367 | -53.728 | â | -0.24 | 0.53 | -32.47 |
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 | 1.14 | 0.65 | 0.22 | 1510 | -0.030 | 712 | 0.62 | 0.02 |
| Li et al. | 2025 | 1.13 | 0.92 | â | 1892 | -0.235 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.190(5) | â | â | â |
| Wei et al. | 2025 | 1.51 | 0.64 | â | 1260 | 0.500 | 712 | 0.50 | â |
| Almeida et al. | 2025 | 1.14 | 0.91 | â | 1914 | â | 938 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1169(1) | â | â |
| Cavallo et al. | 2024 | 1.19 | 0.88 | â | 1445 | 0.160 | â | â | â |
| Hunt & Reffert | 2023 | 1.12 | 0.53 | 0.22 | 1629 | â | â | â | â |
| Almeida et al. | 2023 | 1.14 | 1.08 | â | 1858 | -0.228 | 1689(1) | 0.62 | â |
| Cordoni et al. | 2023 | 1.14 | 0.91 | â | 1914 | -0.089 | 385 | 0.65 | 0.02 |
| Just et al. | 2023 | â | â | â | 1905 | â | 84 | â | â |
| He et al. | 2022 | â | 0.80 | â | 1778 | â | â | â | â |
| Tarricq et al. | 2022 | 1.18 | â | â | 1479 | â | â | â | â |
| Dias et al. | 2021 | 1.14 | 0.91 | â | 1914 | -0.089 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.21 | 0.66 | â | 1413 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.16 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 1510 | 0.000 | â | â | â |
| Bossini et al. | 2019 | 1.17 | 0.63 | â | 1671 | -0.010 | â | â | â |
| Soubiran et al. | 2018 | 1.16 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.16 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.96 | 0.65 | â | 1183 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.93 | 0.64 | â | 1905 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.93 | 0.64 | â | 1905 | -0.030 | â | â | â |
| Gozha et al. | 2012 | 0.94 | â | â | 1172 | -0.030 | 14 | â | â |
| Piskunov et al. | 2008 | 0.94 | 0.65 | â | 1175 | â | â | â | â |
| van den Bergh | 2006 | 0.94 | 0.65 | â | 1175 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.94 | 0.65 | â | 1175 | â | â | â | â |
| Chen et al. | 2003 | 0.94 | 0.65 | â | 1170 | -0.030(1) | â | â | â |
| Dias et al. | 2002 | 0.94 | 0.65 | â | 1172 | -0.030 | 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: intermediate fit.
Cavallo et al. (2024)
Gold sample.