Collinder 308
(NGC 6178; MWSC 2428; OCL 980; ESO 276 06)
0.90
UTI
0.76
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
20.4 [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 308 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young 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 | 248.936 | -45.628 | 1.113 | 0.444 | -3.367 | -9.156 |
| Li et al. | 2025 | 248.939 | -45.635 | 1.099 | 0.521 | -3.342 | â |
| Wei et al. | 2025 | 248.951 | -45.549 | 1.124 | 0.436 | -3.329 | â |
| Almeida et al. | 2025 | 248.933 | -45.646 | â | â | â | â |
| Alfonso et al. | 2024 | 249.034 | -45.413 | 1.072 | 0.433 | -3.306 | â |
| Hunt & Reffert | 2024 | 248.929 | -45.651 | 1.095 | 0.511 | -3.27 | -7.493 |
| Celli et al. | 2024 | 248.939 | -45.635 | â | â | â | â |
| Cavallo et al. | 2024 | 249.082 | -45.453 | 1.098 | â | â | â |
| Hunt & Reffert | 2023 | 248.929 | -45.651 | 1.095 | 0.511 | -3.27 | -7.493 |
| Almeida et al. | 2023 | 248.934 | -45.641 | â | â | â | â |
| Just et al. | 2023 | 248.936 | -45.625 | â | â | â | â |
| He et al. | 2022 | 248.931 | -45.637 | 1.111 | 0.412 | -3.374 | â |
| Jaehnig et al. | 2021 | 248.927 | -45.621 | 1.15 | 0.488 | -3.327 | â |
| Rain et al. | 2021 | 248.939 | -45.635 | 1.099 | 0.521 | -3.342 | â |
| Dias et al. | 2021 | 248.933 | -45.646 | 1.091 | 0.436 | -3.316 | â |
| Cantat-Gaudin et al. | 2020 | 248.939 | -45.635 | 1.099 | 0.521 | -3.342 | â |
| Cantat-Gaudin & Anders | 2020 | 248.939 | -45.635 | 1.099 | 0.521 | -3.342 | â |
| Bica et al. | 2019 | 248.942 | -45.647 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 248.939 | -45.635 | 1.099 | 0.521 | -3.342 | â |
| Loktin & Popova | 2017 | 248.94 | -45.644 | â | -0.74 | -3.699 | 3.5 |
| Kharchenko et al. | 2016 | 248.936 | -45.625 | â | â | â | â |
| Dias et al. | 2014 | 248.946 | -45.643 | â | -0.79 | -0.82 | â |
| Kharchenko et al. | 2013 | 248.947 | -45.625 | â | 0.38 | -3.6 | 3.5 |
| Gozha et al. | 2012 | 248.946 | -45.643 | â | â | â | â |
| Piskunov et al. | 2008 | 248.931 | -45.641 | â | â | â | â |
| Kharchenko et al. | 2007 | 248.94 | -45.64 | â | 0.16 | â | 3.54 |
| van den Bergh | 2006 | 248.95 | -45.633 | â | â | â | â |
| Kharchenko et al. | 2005 | 248.94 | -45.64 | â | 1.17 | -2.04 | 3.54 |
| Kharchenko et al. | 2003 | 248.94 | -45.63 | â | 0.53 | -3.13 | â |
| Chen et al. | 2003 | 248.953 | -45.654 | â | 0.62 | -2.06 | 4.5 |
| Dias et al. | 2002 | 248.946 | -45.643 | â | 0.62 | -2.06 | 3.55 |
| Dambis | 1999 | 248.946 | -45.643 | â | â | â | â |
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 | 0.92 | 0.715 | 1.8 | 17 | 0.013 | 138 | 0.535 | 0.0 |
| Li et al. | 2025 | 0.75 | 0.72 | â | 16 | -0.273 | â | â | â |
| Wei et al. | 2025 | 0.93 | 1.30 | â | 6 | 0.000 | 381 | 0.64 | â |
| Almeida et al. | 2025 | 0.84 | 0.84 | â | 13 | â | 131 | â | â |
| Alfonso et al. | 2024 | 0.91 | 0.52 | â | 17 | 0.068 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 406(1) | â | â |
| Celli et al. | 2024 | â | â | â | 17 | â | 176 | â | â |
| Cavallo et al. | 2024 | 0.93 | 1.21 | â | 6 | -0.100 | â | â | â |
| Hunt & Reffert | 2023 | 0.87 | 0.79 | 1.80 | 8 | â | â | â | â |
| Almeida et al. | 2023 | 0.85 | 0.87 | â | 13 | 0.026 | 122(1) | 0.43 | â |
| Just et al. | 2023 | â | â | â | 32 | â | 60 | â | â |
| He et al. | 2022 | â | 0.85 | â | 8 | â | â | â | â |
| Jaehnig et al. | 2021 | 0.87(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 0.89 | 0.65 | â | 17 | â | â | â | 0 |
| Dias et al. | 2021 | 0.84 | 0.84 | â | 13 | 0.068 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.91 | 0.52 | â | 17 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.89 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.89 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.01 | 0.68 | â | 17 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.01 | 0.74 | â | 32 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.01 | 0.74 | â | 32 | â | â | â | â |
| Gozha et al. | 2012 | 1.01 | â | â | 18 | â | 138 | â | â |
| Piskunov et al. | 2008 | 1.01 | 0.68 | â | 32 | â | â | â | â |
| van den Bergh | 2006 | 1.01 | 0.68 | â | 18 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.01 | 0.68 | â | 32 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.01 | 0.68 | â | â | â | â | â | â |
| Chen et al. | 2003 | 1.01 | â | â | 10 | â | â | â | â |
| Dias et al. | 2002 | 1.01 | 0.68 | â | 18 | â | â | â | â |
| Dambis | 1999 | 0.88 | 0.71 | â | 50 | 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.