Alessi Teutsch 8
(ASCC 68; MWSC 1993; AT 8; FoF 2239)
0.90
UTI
0.83
CN
1.0
Cdens
1.0
CC3
0.84
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 0.84 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 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 |
| Richer et al. | 2021 | 180.634 | -60.895 | 0.957 | -6.626 | 1.617 | 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 |
| Dib et al. | 2018 | 180.712 | -60.92 | â | â | â | â |
| Loktin & Popova | 2017 | 180.735 | -60.924 | â | -3.579 | -1.817 | â |
| Sampedro et al. | 2017 | 180.729 | -60.925 | -4.61 | -0.53 | â | â |
| Joshi et al. | 2016 | 180.712 | -60.92 | â | â | â | 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 | 0.955 | 0.49 | 0.78 | 200 | 0.250 | 847 | 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 |
| Richer et al. | 2021 | â | 0.68 | â | 200 | 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 |
| Kounkel et al. | 2020 | 1.01 | 0.67 | â | 89 | 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 |
| Dib et al. | 2018 | 0.92 | â | â | 398 | â | â | â | â |
| Loktin & Popova | 2017 | 0.77 | 0.62 | â | 184 | â | â | â | â |
| Joshi et al. | 2016 | 0.92 | 0.30 | â | 398 | â | 46 | â | â |
| Kharchenko et al. | 2016 | 0.92 | 0.30 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.92 | 0.30 | â | 398 | â | â | â | â |
| Piskunov et al. | 2008 | 0.65 | 0.32 | â | 447 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.65 | 0.32 | â | 447 | â | â | â | â |
| Dias et al. | 2002 | 0.65 | 0.32 | 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.
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).
Richer et al. (2021)
The expected number of WDs is 23.2, 0 WD candidates found, and 0 WD candidates found in the wide search.
Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010). List of clusters and alike reported by B. Alessi. The Preliminary Amateur Open Cluster Catalog, Version 08/03/2003.