Collinder 307
(MWSC 2427; FoF 863)
0.91
UTI
0.81
CN
1.0
Cdens
1.0
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
3.9 [arcmin]
- CN 0.81 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
Collinder 307 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 moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is well-studied in the literature.
Relatively close
Moderate extinction
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 | 248.785 | -50.989 | 0.506 | -0.761 | -3.324 | -41.949 |
| Almeida et al. | 2025 | 248.794 | -50.989 | β | β | β | β |
| Hunt & Reffert | 2024 | 248.793 | -50.985 | 0.508 | -0.763 | -3.331 | -35.337 |
| Cavallo et al. | 2024 | 248.788 | -50.984 | 0.511 | β | β | β |
| Hunt & Reffert | 2023 | 248.793 | -50.985 | 0.508 | -0.763 | -3.331 | -35.337 |
| Almeida et al. | 2023 | 248.792 | -50.999 | β | β | β | β |
| Just et al. | 2023 | 248.822 | -50.989 | β | β | β | β |
| Dias et al. | 2021 | 248.794 | -50.989 | 0.482 | -0.713 | -3.33 | β |
| Cantat-Gaudin et al. | 2020 | 248.792 | -50.99 | 0.484 | -0.715 | -3.339 | β |
| SΓ‘nchez et al. | 2020 | 248.833 | -51.0 | β | -0.704 | -3.032 | β |
| Cantat-Gaudin & Anders | 2020 | 248.792 | -50.99 | 0.484 | -0.715 | -3.339 | β |
| Liu & Pang | 2019 | 248.808 | -50.999 | 0.491 | -0.741 | -3.316 | β |
| Cantat-Gaudin et al. | 2018 | 248.792 | -50.99 | 0.484 | -0.715 | -3.339 | β |
| Kharchenko et al. | 2016 | 248.822 | -50.989 | β | β | β | β |
| Dias et al. | 2014 | 248.833 | -51.0 | β | -0.55 | -3.5 | β |
| Kharchenko et al. | 2013 | 248.833 | -50.99 | β | -3.41 | -0.04 | β |
| Dias et al. | 2002 | 248.833 | -51.0 | β | -0.65 | -3.69 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 1.68 | 2.55 | β | 82 | β | 764 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1707* | β | β |
| Cavallo et al. | 2024 | 2.23 | 2.72 | β | 257 | 0.830 | β | β | β |
| Hunt & Reffert | 2023 | 1.84 | 2.71 | 1.89 | 187 | β | β | β | β |
| Almeida et al. | 2023 | 1.70 | 2.59 | β | 142 | 0.171 | 713* | 0.61 | β |
| Just et al. | 2023 | β | β | β | 18 | β | 211 | β | β |
| Dias et al. | 2021 | 1.68 | 2.55 | β | 82 | 0.203 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.10 | 2.11 | β | 245 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.95 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 576 | 0.250 | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.95 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 2.06 | 3.61 | β | 18 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.06 | 3.61 | β | 18 | β | β | β | β |
| Dias et al. | 2002 | 1.55 | 2.57 | β | 251 | β | 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: good fit. Gold sample.
Cavallo et al. (2024)
Gold sample.