Haffner 12
(NGC 2425; MWSC 1291; OCL 599; FSR 1238; FoF 377)
0.95
UTI
1.0
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
36.1 [N/pc2]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Haffner 12 is a very rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a massive, near-solar metallicity, old cluster (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 | 99999β | 114.578 | -14.888 | 0.292 | -3.558 | 2.006 | 103.432 |
| Li et al. | 2025 | 114.577 | -14.885 | 0.257 | -3.571 | 2.004 | β |
| Hu & Soubiran | 2025 | 114.575 | -14.88 | β | β | β | β |
| Almeida et al. | 2025 | 114.572 | -14.883 | β | β | β | β |
| Hunt & Reffert | 2024 | 114.58 | -14.888 | 0.284 | -3.573 | 2.011 | 103.907 |
| Cavallo et al. | 2024 | 114.575 | -14.88 | 0.285 | β | β | β |
| Hunt & Reffert | 2023 | 114.58 | -14.888 | 0.284 | -3.573 | 2.011 | 103.907 |
| Just et al. | 2023 | 114.556 | -14.878 | β | β | β | β |
| Dias et al. | 2021 | 114.572 | -14.883 | 0.254 | -3.561 | 1.997 | 103.045 |
| Cantat-Gaudin et al. | 2020 | 114.577 | -14.885 | 0.257 | -3.571 | 2.004 | β |
| SΓ‘nchez et al. | 2020 | 114.571 | -14.878 | β | -3.53 | 1.837 | β |
| Cantat-Gaudin & Anders | 2020 | 114.577 | -14.885 | 0.257 | -3.571 | 2.004 | β |
| Liu & Pang | 2019 | 114.572 | -14.881 | 0.272 | -3.571 | 1.987 | β |
| Bossini et al. | 2019 | 114.577 | -14.885 | β | β | β | β |
| Soubiran et al. | 2018 | 114.577 | -14.885 | β | β | β | 103.13 |
| Bica et al. | 2019 | 114.576 | -14.882 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 114.577 | -14.885 | 0.257 | -3.571 | 2.004 | β |
| Loktin & Popova | 2017 | 114.57 | -14.892 | β | -3.127 | 0.186 | 102.9 |
| Kharchenko et al. | 2016 | 114.556 | -14.878 | β | β | β | β |
| Dias et al. | 2014 | 114.571 | -14.878 | β | -2.7 | 1.0 | β |
| Kharchenko et al. | 2013 | 114.562 | -14.88 | β | -2.86 | 0.61 | 102.9 |
| Gozha et al. | 2012 | 114.571 | -14.878 | β | β | β | β |
| van den Bergh | 2006 | 114.575 | -14.867 | β | β | β | β |
| Dias et al. | 2002 | 114.571 | -14.878 | β | -2.7 | 1.0 | 102.9 |
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 | 3.5 | 0.84 | 0.23 | 2188 | -0.071 | 1824 | β | β |
| Li et al. | 2025 | 3.17 | 0.99 | β | 2670 | -0.071 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.200(5) | β | β | β |
| Almeida et al. | 2025 | 2.71 | 0.84 | β | 4018 | β | 1294 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 3156(1) | β | β |
| Cavallo et al. | 2024 | 2.62 | 1.19 | β | 2818 | -0.210 | β | β | β |
| Hunt & Reffert | 2023 | 3.15 | 0.83 | 0.23 | 1977 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 2188 | β | 1824 | β | β |
| Dias et al. | 2021 | 2.71 | 0.84 | β | 4018 | 0.047 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 3.58 | 0.89 | β | 2399 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.50 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 2950 | 0.000 | β | β | β |
| Bossini et al. | 2019 | 3.38 | 0.88 | β | 2153 | -0.150 | β | β | β |
| Soubiran et al. | 2018 | 3.50 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.50 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 3.97 | 0.84 | β | 2239 | β | β | β | β |
| Kharchenko et al. | 2016 | 4.33 | 0.65 | β | 2188 | β | β | β | β |
| Kharchenko et al. | 2013 | 4.33 | 0.65 | β | 2188 | 0.000 | β | β | β |
| Gozha et al. | 2012 | 3.55 | β | β | 2188 | 0.000 | β | β | β |
| van den Bergh | 2006 | 4.05 | 0.96 | β | 1585 | β | β | β | β |
| Dias et al. | 2002 | 3.55 | 0.65 | β | 2188 | -0.150 | 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. Gold sample.
Cavallo et al. (2024)
Gold sample.