Collinder 268
(VDBH 145; FSR 1644; MWSC 2103; Harvard 8; OCL 895; vdBergh-Hagen 145; ESO 096 06; MWSC 2102; FoF 65)
0.96
UTI
0.79
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
27.7 [N/pc2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Collinder 268 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate 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 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 | 99999β | 199.53 | -67.077 | 0.38 | -5.506 | -0.37 | 21.742 |
| Li et al. | 2025 | 199.543 | -67.079 | 0.357 | -5.48 | -0.405 | β |
| Almeida et al. | 2025 | 199.54 | -67.078 | β | β | β | β |
| Hunt & Reffert | 2024 | 199.544 | -67.084 | 0.385 | -5.506 | -0.371 | -50.71 |
| Cavallo et al. | 2024 | 199.53 | -67.077 | 0.385 | β | β | β |
| Hunt & Reffert | 2023 | 199.544 | -67.084 | 0.385 | -5.506 | -0.371 | -50.71 |
| Just et al. | 2023 | 199.556 | -67.072 | β | β | β | β |
| Jaehnig et al. | 2021 | 199.548 | -67.079 | 0.38 | -5.463 | -0.401 | β |
| Rain et al. | 2021 | 199.543 | -67.079 | 0.357 | -5.48 | -0.405 | β |
| Dias et al. | 2021 | 199.54 | -67.078 | 0.359 | -5.49 | -0.403 | β |
| Cantat-Gaudin et al. | 2020 | 199.543 | -67.079 | 0.357 | -5.48 | -0.405 | β |
| SΓ‘nchez et al. | 2020 | 199.554 | -67.083 | β | -5.662 | -0.462 | β |
| Cantat-Gaudin & Anders | 2020 | 199.543 | -67.079 | 0.357 | -5.48 | -0.405 | β |
| Liu & Pang | 2019 | 199.503 | -67.077 | 0.363 | -5.481 | -0.457 | β |
| Bossini et al. | 2019 | 199.543 | -67.079 | β | β | β | β |
| Soubiran et al. | 2018 | 199.543 | -67.079 | β | β | β | -34.35 |
| Bica et al. | 2019 | 199.467 | -67.059 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 199.543 | -67.079 | 0.357 | -5.48 | -0.405 | β |
| Loktin & Popova | 2017 | 199.56 | -67.083 | β | -3.913 | -2.3 | -27.2 |
| Kharchenko et al. | 2016 | 199.556 | -67.072 | β | β | β | β |
| Dias et al. | 2014 | 199.554 | -67.083 | β | -2.12 | -0.46 | β |
| Kharchenko et al. | 2013 | 199.567 | -67.075 | β | -1.2 | 1.92 | -27.2 |
| Gozha et al. | 2012 | 199.554 | -67.083 | β | β | β | β |
| Froebrich et al. | 2007 | 199.475 | -67.058 | β | β | β | β |
| van den Bergh | 2006 | 199.7 | -67.2 | β | β | β | β |
| Dias et al. | 2002 | 199.554 | -67.083 | β | -2.12 | -0.46 | -27.18 |
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 | 2.325 | 1.16 | 0.88 | 419 | 0.075 | 815 | β | 1.0 |
| Li et al. | 2025 | 2.41 | 1.23 | β | 440 | 0.068 | β | β | β |
| Almeida et al. | 2025 | 2.28 | 1.63 | β | 54 | β | 815 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1222(1) | β | β |
| Cavallo et al. | 2024 | 2.23 | 1.42 | β | 398 | 0.080 | β | β | β |
| Hunt & Reffert | 2023 | 2.37 | 1.20 | 0.88 | 254 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 617 | β | 73 | β | β |
| Jaehnig et al. | 2021 | 2.62(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 2.59 | 0.93 | β | 562 | β | β | β | 1 |
| Dias et al. | 2021 | 2.28 | 1.63 | β | 54 | 0.075 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.63 | 1.16 | β | 240 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.59 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 331 | 0.250 | β | β | β |
| Bossini et al. | 2019 | 2.44 | 1.25 | β | 242 | 0.000 | β | β | β |
| Soubiran et al. | 2018 | 2.59 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.59 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.92 | 1.12 | β | 281 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.81 | 1.07 | β | 617 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.81 | 1.07 | β | 617 | β | β | β | β |
| Gozha et al. | 2012 | 1.96 | β | β | 574 | β | β | β | β |
| van den Bergh | 2006 | 1.96 | 0.96 | β | 575 | β | β | β | β |
| Dias et al. | 2002 | 1.96 | 0.95 | β | 574 | 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: good fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.