Alessi Teutsch 3
(ASCC 42; MWSC 1373; AT 3; Alessi 30)
0.95
UTI
0.76
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
8.2 [N/pc2]
- CN 0.76 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 3 is a rich, very dense object of very 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, intermediate-age cluster (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 | 118.295 | -53.023 | 1.423 | -5.389 | 8.937 | 9.545 |
| Li et al. | 2025 | 118.228 | -53.022 | 1.417 | -5.378 | 8.926 | â |
| Wei et al. | 2025 | 118.212 | -53.025 | 1.43 | -5.377 | 8.949 | â |
| Almeida et al. | 2025 | 118.237 | -53.053 | â | â | â | â |
| Alfonso et al. | 2024 | 118.167 | -52.972 | 1.382 | -5.309 | 8.906 | â |
| Hunt & Reffert | 2024 | 118.286 | -53.001 | 1.421 | -5.338 | 8.945 | 10.654 |
| Cavallo et al. | 2024 | 118.227 | -53.048 | 1.422 | â | â | â |
| Hunt & Reffert | 2023 | 118.286 | -53.001 | 1.421 | -5.338 | 8.945 | 10.654 |
| Almeida et al. | 2023 | 118.25 | -52.99 | â | â | â | â |
| Just et al. | 2023 | 118.136 | -52.992 | â | â | â | â |
| He et al. | 2022 | 118.251 | -53.032 | 1.426 | -5.379 | 8.962 | â |
| Tarricq et al. | 2022 | 118.303 | -53.011 | 1.428 | -5.377 | 8.919 | â |
| Dias et al. | 2021 | 118.237 | -53.053 | 1.423 | -5.364 | 8.908 | 17.865 |
| Cantat-Gaudin et al. | 2020 | 118.228 | -53.022 | 1.417 | -5.378 | 8.926 | â |
| Cantat-Gaudin & Anders | 2020 | 118.228 | -53.022 | 1.417 | -5.378 | 8.926 | â |
| Bossini et al. | 2019 | 118.228 | -53.022 | â | â | â | â |
| Soubiran et al. | 2018 | 118.228 | -53.022 | â | â | â | 16.59 |
| Bica et al. | 2019 | 118.253 | -53.051 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 118.228 | -53.022 | 1.417 | -5.378 | 8.926 | â |
| Loktin & Popova | 2017 | 118.26 | -53.044 | â | -1.918 | 8.792 | 15.0 |
| Kharchenko et al. | 2016 | 118.136 | -52.992 | â | â | â | â |
| Dias et al. | 2014 | 118.254 | -53.045 | â | -4.23 | 5.11 | â |
| Kharchenko et al. | 2013 | 118.14 | -52.995 | â | -3.67 | 8.21 | â |
| Piskunov et al. | 2008 | 118.215 | -53.008 | â | â | â | â |
| Kharchenko et al. | 2005 | 118.21 | -53.01 | â | -3.76 | 8.25 | â |
| Dias et al. | 2002 | 118.254 | -53.045 | â | -4.23 | 5.11 | 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 | 0.69 | 0.52 | 1.09 | 141 | 0.011 | 209 | 0.355 | â |
| Li et al. | 2025 | 0.70 | 0.60 | â | 104 | 0.059 | â | â | â |
| Wei et al. | 2025 | 0.86 | 0.77 | â | 54 | 0.000 | 270 | 0.29 | â |
| Almeida et al. | 2025 | 0.69 | 0.70 | â | 160 | â | 209 | â | â |
| Alfonso et al. | 2024 | 0.69 | 0.47 | â | 107 | 0.011 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 151(1) | â | â |
| Cavallo et al. | 2024 | 0.71 | 0.74 | â | 115 | 0.210 | â | â | â |
| Hunt & Reffert | 2023 | 0.67 | 0.51 | 1.09 | 103 | â | â | â | â |
| Almeida et al. | 2023 | 0.68 | 0.74 | â | 149 | -0.039 | 235(1) | 0.42 | â |
| Just et al. | 2023 | â | â | â | 141 | â | 28 | â | â |
| He et al. | 2022 | â | 0.80 | â | 79 | â | â | â | â |
| Tarricq et al. | 2022 | 0.68 | â | â | 115 | â | â | â | â |
| Dias et al. | 2021 | 0.69 | 0.70 | â | 160 | 0.011 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.69 | 0.47 | â | 105 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.69 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 0.66 | 0.42 | â | 97 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.69 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.69 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.88 | 0.74 | â | 618 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.79 | 0.52 | â | 141 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.79 | 0.52 | â | 141 | â | â | â | â |
| Piskunov et al. | 2008 | 0.80 | 0.31 | â | 372 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.80 | 0.31 | â | 372 | â | â | â | â |
| Dias et al. | 2002 | 0.80 | 0.31 | â | 372 | 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: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.