Haffner 6
(MWSC 1177; OCL 582)
0.94
UTI
0.86
CN
0.89
Cdens
1.0
CC3
0.97
Clit
1.0
Cdup
Nm (P>50%)
386
Core radius and density
2.2 [pc], 4.5 [pc-2]
- CN 0.86 Rich
- Cdens 0.89 Dense
- CC3 1.0 Very high quality
- Clit 0.97 Very well-studied
- Cdup 1.0 Unique
Overview
Haffner 6 is a rich, dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity 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 | 99999â | 109.991 | -13.153 | 0.2 | -1.261 | 2.004 | 71.116 |
| Otto et al. | 2026 | 109.991 | -13.152 | â | -1.22 | 1.96 | 70.0 |
| Li et al. | 2025 | 109.998 | -13.151 | 0.204 | -1.22 | 1.96 | â |
| Hu & Soubiran | 2025 | 109.986 | -13.152 | â | â | â | â |
| Almeida et al. | 2025 | 109.998 | -13.153 | â | â | â | â |
| Hunt & Reffert | 2024 | 109.991 | -13.152 | 0.206 | -1.253 | 2.0 | 84.394 |
| Cavallo et al. | 2024 | 109.986 | -13.152 | 0.204 | â | â | â |
| Hunt & Reffert | 2023 | 109.991 | -13.152 | 0.206 | -1.253 | 2.0 | 84.394 |
| Almeida et al. | 2023 | 109.998 | -13.152 | â | â | â | â |
| Just et al. | 2023 | 110.009 | -13.148 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 109.998 | -13.151 | â | â | â | â |
| Jaehnig et al. | 2021 | 109.997 | -13.152 | 0.223 | -1.223 | 1.949 | â |
| Rain et al. | 2021 | 109.998 | -13.151 | 0.204 | -1.22 | 1.96 | â |
| Dias et al. | 2021 | 109.998 | -13.153 | 0.212 | -1.226 | 1.964 | 69.56 |
| Cantat-Gaudin et al. | 2020 | 109.998 | -13.151 | 0.204 | -1.22 | 1.96 | â |
| Cantat-Gaudin & Anders | 2020 | 109.998 | -13.151 | 0.204 | -1.22 | 1.96 | â |
| Bossini et al. | 2019 | 109.998 | -13.151 | â | â | â | â |
| Soubiran et al. | 2018 | 109.998 | -13.151 | â | â | â | 70.03 |
| Bica et al. | 2019 | 109.999 | -13.146 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 109.998 | -13.151 | 0.204 | -1.22 | 1.96 | â |
| Dias et al. | 2018 | â | â | â | -2.4 | 2.04 | â |
| Loktin & Popova | 2017 | 110.025 | -13.15 | â | -0.749 | 3.885 | â |
| Sampedro et al. | 2017 | 110.025 | -13.133 | â | -0.04 | 4.39 | â |
| Kharchenko et al. | 2016 | 110.009 | -13.148 | â | â | â | â |
| Dias et al. | 2014 | 110.025 | -13.133 | â | -0.55 | 3.58 | â |
| Kharchenko et al. | 2013 | 110.014 | -13.15 | â | 0.36 | 4.16 | â |
| Bukowiecki et al. | 2011 | 110.004 | -13.154 | â | â | â | â |
| Ahumada & Lapasset | 2007 | 110.025 | -13.133 | â | â | â | â |
| van den Bergh | 2006 | 109.988 | -13.161 | â | â | â | â |
| Dias et al. | 2002 | 110.025 | -13.133 | â | -0.55 | 3.58 | â |
| Lynga | 1987 | 110.013 | -13.128 | 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 | 4.11 | 1.63 | 1.56 | 644 | -0.219 | 1909 | 0.63 | 1 |
| Otto et al. | 2026 | â | â | â | 617 | -0.250(15) | â | â | â |
| Li et al. | 2025 | 4.67 | 1.74 | â | 656 | 0.052 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.280(5) | â | â | â |
| Almeida et al. | 2025 | 3.86 | 1.94 | â | 684 | â | 1696 | â | â |
| Hunt & Reffert | 2024 | 4.42 | 1.63 | 1.56 | 439 | â | 2806(1) | â | â |
| Cavallo et al. | 2024 | 3.27 | 2.14 | â | 603 | -0.510 | â | â | â |
| Hunt & Reffert | 2023 | 4.42 | 1.63 | 1.56 | 439 | â | â | â | â |
| Almeida et al. | 2023 | 4.11 | 2.08 | â | 430 | -0.219 | 1745(1) | 0.63 | â |
| Just et al. | 2023 | â | â | â | 733 | â | 733 | â | â |
| Jadhav & Subramaniam | 2021 | 4.47 | 1.36 | â | 617 | â | 2073 | â | 0(1) |
| Jaehnig et al. | 2021 | 4.43(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 4.29 | 1.42 | â | 661 | â | â | â | 1 |
| Dias et al. | 2021 | 3.86 | 1.94 | â | 684 | -0.183 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 4.47 | 1.36 | â | 617 | â | â | â | â |
| Kounkel et al. | 2020 | 3.87 | 1.64 | â | 501 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.29 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 4.29 | 1.46 | â | 542 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 4.29 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.29 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.21 | 2.66 | â | 81 | â | â | â | â |
| Kharchenko et al. | 2016 | 3.32 | 1.91 | â | 733 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.32 | 1.91 | â | 733 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 3047 | â | â |
| Bukowiecki et al. | 2011 | 3.78(1) | 1.58 | â | 631 | â | â | â | â |
| Ahumada & Lapasset | 2007 | â | 1.42 | â | 676 | â | â | â | 2 |
| van den Bergh | 2006 | 3.05 | 1.42 | â | 676 | â | â | â | â |
| Dias et al. | 2002 | 3.05 | 1.42 | â | 670 | â | â | â | â |
| Lynga | 1987 | 1.10 | 0.00 | â | 794 | 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: good fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.0862, e_all=0.1291.