Haffner 8
(OCL 578; MWSC 1200; FoF 376)
0.87
UTI
0.84
CN
1.0
Cdens
0.75
CC3
0.87
Clit
1.0
Cdup
Nm (P>50%)
342
Core radius and density
2.0 [pc], 8.0 [pc-2]
- CN 0.84 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.87 Well-studied
- Cdup 1.0 Unique
Overview
Haffner 8 is a 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 near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the absorption and metallicity parameters (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 | 99999â | 110.771 | -12.307 | 0.326 | -1.611 | 0.474 | 58.585 |
| Li et al. | 2025 | 110.777 | -12.31 | 0.314 | -1.626 | 0.446 | â |
| Almeida et al. | 2025 | 110.784 | -12.315 | â | â | â | â |
| Hunt & Reffert | 2024 | 110.772 | -12.303 | 0.335 | -1.62 | 0.475 | 57.369 |
| Cavallo et al. | 2024 | 110.772 | -12.309 | 0.333 | â | â | â |
| Hunt & Reffert | 2023 | 110.772 | -12.303 | 0.335 | -1.62 | 0.475 | 57.369 |
| Almeida et al. | 2023 | 110.776 | -12.319 | â | â | â | â |
| Jaehnig et al. | 2021 | 110.768 | -12.309 | 0.352 | -1.608 | 0.425 | â |
| Rain et al. | 2021 | 110.777 | -12.31 | 0.314 | -1.626 | 0.446 | â |
| Dias et al. | 2021 | 110.784 | -12.315 | 0.311 | -1.634 | 0.448 | 61.879 |
| Cantat-Gaudin et al. | 2020 | 110.777 | -12.31 | 0.314 | -1.626 | 0.446 | â |
| Cantat-Gaudin & Anders | 2020 | 110.777 | -12.31 | 0.314 | -1.626 | 0.446 | â |
| Liu & Pang | 2019 | 110.771 | -12.322 | 0.317 | -1.598 | 0.456 | â |
| Soubiran et al. | 2018 | 110.777 | -12.31 | â | â | â | 61.49 |
| Bica et al. | 2019 | 110.765 | -12.294 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 110.777 | -12.31 | 0.314 | -1.626 | 0.446 | â |
| Dias et al. | 2018 | â | â | â | -2.34 | 0.97 | â |
| Dib et al. | 2018 | 110.793 | -12.308 | â | â | â | â |
| Sampedro et al. | 2017 | 110.85 | -12.333 | â | -3.68 | -0.58 | â |
| Joshi et al. | 2016 | 110.793 | -12.308 | â | â | â | â |
| Dias et al. | 2014 | 110.85 | -12.333 | â | -3.6 | -0.73 | â |
| Gozha et al. | 2012 | 110.85 | -12.333 | â | â | â | â |
| Bukowiecki et al. | 2011 | 110.763 | -12.303 | â | â | â | â |
| Ahumada & Lapasset | 2007 | 110.85 | -12.333 | â | â | â | â |
| van den Bergh | 2006 | 110.85 | -12.333 | â | â | â | â |
| Dias et al. | 2002 | 110.85 | -12.333 | â | -3.6 | -0.73 | â |
| Lynga | 1987 | 110.84 | -12.324 | 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 | 2.62 | 0.91 | 0.71 | 340 | 0.040 | 732 | 0.52 | 0 |
| Li et al. | 2025 | 2.87 | 1.17 | â | 288 | 0.138 | â | â | â |
| Almeida et al. | 2025 | 2.51 | 1.29 | â | 286 | â | 553 | â | â |
| Hunt & Reffert | 2024 | 2.62 | 0.91 | 0.71 | 341 | â | 830(1) | â | â |
| Cavallo et al. | 2024 | 3.03 | 1.30 | â | 302 | 0.540 | â | â | â |
| Hunt & Reffert | 2023 | 2.62 | 0.91 | 0.71 | 340 | â | â | â | â |
| Almeida et al. | 2023 | 2.50 | 1.29 | â | 340 | -0.116 | 633(1) | 0.52 | â |
| Jaehnig et al. | 2021 | 2.84(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 2.91 | 0.09 | â | 316 | â | â | â | 0 |
| Dias et al. | 2021 | 2.51 | 1.29 | â | 286 | -0.078 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.01 | 1.16 | â | 240 | â | â | â | â |
| Kounkel et al. | 2020 | 2.93 | 1.37 | â | 339 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.91 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 63 | 0.500 | â | â | â |
| Soubiran et al. | 2018 | 2.91 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.91 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.20 | â | â | 1084 | â | â | â | â |
| Joshi et al. | 2016 | 1.20 | 0.09 | â | 1084 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 1145 | â | â |
| Gozha et al. | 2012 | 1.18 | â | â | 1413 | 0.020 | â | â | â |
| Bukowiecki et al. | 2011 | 3.24(1) | 0.47 | â | 794 | â | â | â | â |
| Paunzen et al. | 2010 | â | â | â | â | 0.020 | â | â | â |
| Ahumada & Lapasset | 2007 | â | 0.09 | â | 1413 | â | â | â | 0 |
| van den Bergh | 2006 | 1.18 | 0.09 | â | 1413 | â | â | â | â |
| Dias et al. | 2002 | 2.38 | 0.10 | â | 316 | 0.060 | â | â | â |
| Lynga | 1987 | 1.70 | 0.00 | â | 501 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P120, along with OC_0382.
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good 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=0.1584, e_all=0.1043.