Collinder 278
(VDBH 153; NGC 5288; OCL 910; vdBergh-Hagen 153; ESO 097 07; MWSC 2168; FoF 138)
0.91
UTI
0.79
CN
1.0
Cdens
1.0
CC3
0.87
Clit
1.0
Cdup
Stellar density (N50/rad)
46.0 [N/pc2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.87 Well-studied
- Cdup 1.0 Unique
π₯ Members
π Colab
π¬ Bayestar19
MOCA
π CDS
π Simbad
π CDS (Ξ±, Ξ΄)
π Simbad (Ξ±, Ξ΄)
MOCA
π CDS
π Simbad
π CDS (Ξ±, Ξ΄)
π Simbad (Ξ±, Ξ΄)
Overview
Collinder 278 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 metallicity parameter (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 207.196 | -64.675 | 0.379 | -3.866 | -1.905 | -20.997 |
| Li et al. | 2025 | 207.193 | -64.68 | 0.345 | -3.85 | -1.935 | β |
| Hu & Soubiran | 2025 | 207.187 | -64.68 | β | β | β | β |
| Almeida et al. | 2025 | 207.189 | -64.679 | β | β | β | β |
| Hunt & Reffert | 2024 | 207.2 | -64.671 | 0.383 | -3.85 | -1.902 | -17.803 |
| Cavallo et al. | 2024 | 207.187 | -64.68 | 0.38 | β | β | β |
| Hunt & Reffert | 2023 | 207.2 | -64.671 | 0.383 | -3.85 | -1.902 | -17.803 |
| Almeida et al. | 2023 | 207.188 | -64.676 | β | β | β | β |
| Dias et al. | 2021 | 207.189 | -64.679 | 0.351 | -3.873 | -1.928 | -23.342 |
| Cantat-Gaudin et al. | 2020 | 207.193 | -64.68 | 0.345 | -3.85 | -1.935 | β |
| SΓ‘nchez et al. | 2020 | 207.183 | -64.685 | β | -3.837 | -2.005 | β |
| Cantat-Gaudin & Anders | 2020 | 207.193 | -64.68 | 0.345 | -3.85 | -1.935 | β |
| Liu & Pang | 2019 | 207.203 | -64.673 | 0.345 | -3.841 | -1.905 | β |
| Soubiran et al. | 2018 | 207.193 | -64.68 | β | β | β | -23.83 |
| Bica et al. | 2019 | 207.182 | -64.684 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 207.193 | -64.68 | 0.345 | -3.85 | -1.935 | β |
| Dias et al. | 2014 | 207.183 | -64.685 | β | -5.25 | -5.79 | β |
| Dias et al. | 2002 | 207.183 | -64.685 | β | -5.12 | -5.98 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 2.35 | 1.58 | 1.28 | 387 | 0.225 | 548 | 0.61 | β |
| Li et al. | 2025 | 2.44 | 1.43 | β | 534 | 0.230 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.180(5) | β | β | β |
| Almeida et al. | 2025 | 2.35 | 1.72 | β | 327 | β | 548 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1224(1) | β | β |
| Cavallo et al. | 2024 | 2.04 | 1.43 | β | 631 | 0.220 | β | β | β |
| Hunt & Reffert | 2023 | 2.34 | 1.45 | 1.28 | 337 | β | β | β | β |
| Almeida et al. | 2023 | 2.29 | 1.71 | β | 387 | 0.094 | 475(1) | 0.61 | β |
| Dias et al. | 2021 | 2.35 | 1.72 | β | 327 | 0.318 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.68 | 1.38 | β | 468 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.67 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 562 | 0.500 | β | β | β |
| Soubiran et al. | 2018 | 2.67 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.67 | β | β | β | β | β | β | β |
| Dias et al. | 2002 | 2.16 | 2.02 | β | 178 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Gold sample.
Cavallo et al. (2024)
Gold sample.