Alessi Teutsch 8
(ASCC 68; MWSC 1993; AT 8; FoF 2239)
0.97
UTI
0.83
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
22.9 [N/pc2]
- CN 0.83 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Alessi Teutsch 8 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near 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 age, metallicity, and mass parameters (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 | 99999â | 180.663 | -60.939 | 0.985 | -6.642 | 1.666 | -18.849 |
| Li et al. | 2025 | 180.649 | -60.935 | 0.967 | -6.625 | 1.63 | â |
| Wei et al. | 2025 | 180.635 | -60.935 | 0.99 | -6.645 | 1.681 | â |
| Almeida et al. | 2025 | 180.649 | -60.948 | â | â | â | â |
| Hunt & Reffert | 2024 | 180.703 | -60.953 | 0.989 | -6.645 | 1.672 | -23.68 |
| Cavallo et al. | 2024 | 180.672 | -60.955 | 0.989 | â | â | â |
| Hunt & Reffert | 2023 | 180.703 | -60.953 | 0.989 | -6.645 | 1.672 | -23.68 |
| Just et al. | 2023 | 180.703 | -60.917 | â | â | â | â |
| He et al. | 2022 | 180.662 | -60.938 | 0.991 | -6.64 | 1.681 | â |
| Tarricq et al. | 2022 | 180.671 | -60.902 | 0.982 | -6.647 | 1.667 | â |
| Dias et al. | 2021 | 180.649 | -60.948 | 0.971 | -6.629 | 1.636 | -15.38 |
| Cantat-Gaudin et al. | 2020 | 180.649 | -60.935 | 0.967 | -6.625 | 1.63 | â |
| Cantat-Gaudin & Anders | 2020 | 180.649 | -60.935 | 0.967 | -6.625 | 1.63 | â |
| Liu & Pang | 2019 | 180.66 | -60.94 | 0.972 | -6.611 | 1.627 | â |
| Soubiran et al. | 2018 | 180.649 | -60.935 | â | â | â | -15.35 |
| Bica et al. | 2019 | 180.73 | -60.928 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 180.649 | -60.935 | 0.967 | -6.625 | 1.63 | â |
| Loktin & Popova | 2017 | 180.735 | -60.924 | â | -3.579 | -1.817 | â |
| Kharchenko et al. | 2016 | 180.703 | -60.917 | â | â | â | â |
| Dias et al. | 2014 | 180.729 | -60.925 | â | -4.71 | -0.11 | â |
| Kharchenko et al. | 2013 | 180.712 | -60.92 | â | -4.63 | 3.0 | â |
| Piskunov et al. | 2008 | 180.733 | -60.919 | â | â | â | â |
| Kharchenko et al. | 2005 | 180.73 | -60.92 | â | -4.81 | 3.71 | â |
| Dias et al. | 2002 | 180.729 | -60.925 | â | -4.71 | -0.11 | 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 | 0.96 | 0.485 | 0.78 | 190 | 0.250 | 864 | 0.33 | â |
| Li et al. | 2025 | 0.95 | 0.49 | â | 305 | 0.050 | â | â | â |
| Wei et al. | 2025 | 1.74 | 0.94 | â | 100 | 0.500 | 847 | 0.33 | â |
| Almeida et al. | 2025 | 0.97 | 0.63 | â | 190 | â | 882 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1184(1) | â | â |
| Cavallo et al. | 2024 | 0.98 | 0.47 | â | 372 | 0.400 | â | â | â |
| Hunt & Reffert | 2023 | 0.95 | 0.48 | 0.78 | 134 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 398 | â | 251 | â | â |
| He et al. | 2022 | â | 0.85 | â | 79 | â | â | â | â |
| Tarricq et al. | 2022 | 0.96 | â | â | 115 | â | â | â | â |
| Dias et al. | 2021 | 0.97 | 0.63 | â | 190 | 0.154 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.99 | 0.49 | â | 117 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.00 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 93 | 0.250 | â | â | â |
| Soubiran et al. | 2018 | 1.00 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.00 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.77 | 0.61 | â | 184 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.92 | 0.29 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.92 | 0.29 | â | 398 | â | â | â | â |
| Piskunov et al. | 2008 | 0.65 | 0.31 | â | 447 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.65 | 0.31 | â | 447 | â | â | â | â |
| Dias et al. | 2002 | 0.65 | 0.31 | â | 447 | 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: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.