Alessi Teutsch 12
(ASCC 86; AT 12; Alessi J1701.7-5857; MWSC 2513)
0.85
UTI
0.52
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
5.7 [N/pc2]
- CN 0.52 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Alessi Teutsch 12 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (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 | 255.372 | -58.995 | 1.656 | -2.272 | -8.974 | -2.729 |
| Li et al. | 2025 | 255.421 | -58.981 | 1.632 | -2.134 | -8.952 | â |
| Almeida et al. | 2025 | 255.415 | -59.026 | â | â | â | â |
| Alfonso et al. | 2024 | 255.409 | -59.048 | 1.624 | -2.27 | -8.96 | â |
| Hunt & Reffert | 2024 | 255.411 | -59.008 | 1.644 | -2.313 | -8.985 | -5.207 |
| Cavallo et al. | 2024 | 255.353 | -59.036 | 1.647 | â | â | â |
| Hunt & Reffert | 2023 | 255.411 | -59.008 | 1.644 | -2.313 | -8.985 | -5.207 |
| Tarricq et al. | 2022 | 255.35 | -58.985 | 1.643 | -2.289 | -8.961 | â |
| Dias et al. | 2021 | 255.415 | -59.026 | 1.628 | -2.169 | -8.946 | -11.236 |
| Cantat-Gaudin et al. | 2020 | 255.421 | -58.981 | 1.632 | -2.134 | -8.952 | â |
| Cantat-Gaudin & Anders | 2020 | 255.421 | -58.981 | 1.632 | -2.134 | -8.952 | â |
| Bossini et al. | 2019 | 255.421 | -58.981 | â | â | â | â |
| Soubiran et al. | 2018 | 255.421 | -58.981 | â | â | â | -5.88 |
| Bica et al. | 2019 | 255.438 | -58.957 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 255.421 | -58.981 | 1.632 | -2.134 | -8.952 | â |
| Dias et al. | 2014 | 255.446 | -58.958 | â | -2.72 | -5.32 | â |
| Gozha et al. | 2012 | 255.446 | -58.958 | â | â | â | â |
| Piskunov et al. | 2008 | 255.481 | -59.011 | â | â | â | â |
| Kharchenko et al. | 2007 | 255.49 | -59.01 | â | 0.55 | â | -6.0 |
| Kharchenko et al. | 2005 | 255.49 | -59.01 | â | -3.34 | -7.79 | -6.0 |
| Dias et al. | 2002 | 255.446 | -58.958 | â | -3.34 | -7.79 | -6.0 |
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 | 0.62 | 0.37 | 0.45 | 86 | 0.000 | 88 | â | â |
| Li et al. | 2025 | 0.65 | 0.32 | â | 78 | 0.232 | â | â | â |
| Almeida et al. | 2025 | 0.60 | 0.48 | â | 86 | â | 88 | â | â |
| Alfonso et al. | 2024 | 0.64 | 0.35 | â | 72 | -0.056 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 42(1) | â | â |
| Cavallo et al. | 2024 | 0.61 | 0.42 | â | 110 | 0.460 | â | â | â |
| Hunt & Reffert | 2023 | 0.58 | 0.20 | 0.45 | 105 | â | â | â | â |
| Tarricq et al. | 2022 | 0.63 | â | â | 89 | â | â | â | â |
| Dias et al. | 2021 | 0.60 | 0.48 | â | 86 | -0.056 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.64 | 0.35 | â | 87 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.60 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 0.61 | 0.38 | â | 95 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.60 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.60 | â | â | â | â | â | â | â |
| Gozha et al. | 2012 | 0.70 | â | â | 12 | â | 1047 | â | â |
| Piskunov et al. | 2008 | 0.70 | 0.37 | â | 12 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.70 | 0.37 | â | 12 | â | â | â | â |
| Dias et al. | 2002 | 0.70 | 0.37 | â | 12 | 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: worst fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.