Alessi Teutsch 11
(ASCC 112; MWSC 3295; AT 11; Alessi 46; Alessi J2016.5+5204; FoF 2358)
0.96
UTI
0.82
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
22.8 [N/pc2]
- CN 0.82 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 11 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the 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 | 304.148 | 52.047 | 1.533 | -0.119 | -1.291 | -27.173 |
| Bijavara Seshashayana et al. | 2025 | 304.093 | 52.105 | â | â | â | â |
| Li et al. | 2025 | 304.127 | 52.051 | 1.52 | -0.139 | -1.295 | â |
| Yang et al. | 2025 | 304.102 | 52.074 | â | â | â | â |
| Almeida et al. | 2025 | 304.143 | 52.032 | â | â | â | â |
| Alfonso et al. | 2024 | 304.146 | 52.073 | 1.504 | -0.133 | -1.264 | â |
| Zhang et al. | 2024 | 304.102 | 52.074 | â | â | â | â |
| Hunt & Reffert | 2024 | 304.102 | 52.074 | 1.537 | -0.129 | -1.303 | -27.811 |
| Cavallo et al. | 2024 | 304.087 | 52.056 | 1.534 | â | â | â |
| Hunt & Reffert | 2023 | 304.102 | 52.074 | 1.537 | -0.129 | -1.303 | -27.811 |
| Almeida et al. | 2023 | 304.206 | 52.01 | â | â | â | â |
| Just et al. | 2023 | 304.092 | 52.095 | â | â | â | â |
| He et al. | 2022 | 304.138 | 52.056 | 1.538 | -0.124 | -1.311 | â |
| Tarricq et al. | 2022 | 304.028 | 52.086 | 1.551 | -0.143 | -1.288 | â |
| Dias et al. | 2021 | 304.143 | 52.032 | 1.514 | -0.139 | -1.267 | -25.929 |
| Cantat-Gaudin et al. | 2020 | 304.127 | 52.051 | 1.52 | -0.139 | -1.295 | â |
| Zhong et al. | 2020 | 304.127 | 52.051 | â | -0.139 | -1.295 | -31.98 |
| Cantat-Gaudin & Anders | 2020 | 304.127 | 52.051 | 1.52 | -0.139 | -1.295 | â |
| Liu & Pang | 2019 | 304.141 | 52.057 | 1.52 | -0.153 | -1.222 | â |
| Bossini et al. | 2019 | 304.11 | 52.056 | â | â | â | â |
| Soubiran et al. | 2018 | 304.127 | 52.051 | â | â | â | -26.67 |
| Bica et al. | 2019 | 304.132 | 52.078 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 304.127 | 52.051 | 1.52 | -0.139 | -1.295 | â |
| Dib et al. | 2018 | 304.095 | 52.098 | â | â | â | â |
| Loktin & Popova | 2017 | 304.14 | 52.075 | â | -1.005 | -0.296 | â |
| Sampedro et al. | 2017 | 304.133 | 52.075 | 0.31 | -1.49 | â | â |
| Joshi et al. | 2016 | 304.095 | 52.098 | â | â | â | â |
| Kharchenko et al. | 2016 | 304.092 | 52.095 | â | â | â | â |
| Dias et al. | 2014 | 304.133 | 52.075 | â | -0.06 | -1.46 | â |
| Kharchenko et al. | 2013 | 304.095 | 52.098 | â | -0.33 | -0.31 | â |
| Piskunov et al. | 2008 | 304.113 | 52.097 | â | â | â | â |
| Piskunov et al. | 2007 | 304.113 | 52.097 | â | â | â | â |
| Kharchenko et al. | 2005 | 304.11 | 52.1 | â | -0.37 | -0.73 | â |
| Dias et al. | 2002 | 304.133 | 52.075 | â | -0.06 | -1.46 | 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 | 0.63 | 0.25 | 0.57 | 141 | 0.026 | 48 | 0.51 | â |
| Bijavara Seshashayana et al. | 2025 | â | 0.37 | â | 140 | -0.100(14) | â | â | â |
| Li et al. | 2025 | 0.66 | 0.09 | â | 257 | 0.246 | â | â | â |
| Yang et al. | 2025 | â | â | â | 182 | -0.120(3) | â | â | â |
| Almeida et al. | 2025 | 0.64 | 0.22 | â | 179 | â | 203 | â | â |
| Alfonso et al. | 2024 | 0.63 | 0.37 | â | 98 | 0.070 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.069(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 335(1) | â | â |
| Cavallo et al. | 2024 | 0.66 | 0.46 | â | 79 | 0.190 | â | â | â |
| Hunt & Reffert | 2023 | 0.61 | 0.10 | 0.57 | 180 | â | â | â | â |
| Almeida et al. | 2023 | 0.64 | 0.26 | â | 179 | 0.024 | 217(1) | 0.51 | â |
| Just et al. | 2023 | â | â | â | 141 | â | 14 | â | â |
| He et al. | 2022 | â | 0.45 | â | 112 | â | â | â | â |
| Spina et al. | 2022 | â | â | â | â | -0.182 | â | â | â |
| Tarricq et al. | 2022 | 0.62 | â | â | 155 | â | â | â | â |
| Dias et al. | 2021 | 0.64 | 0.22 | â | 179 | 0.072 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.63 | 0.37 | â | 145 | â | â | â | â |
| Kounkel et al. | 2020 | 0.64 | 0.41 | â | 100 | â | â | â | â |
| Zhong et al. | 2020 | 0.65(1) | 0.32 | â | 8179 | 0.029 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.65 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 105 | 0.250 | â | â | â |
| Bossini et al. | 2019 | 0.63 | 0.31 | â | 152 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.65 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.65 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 0.57 | â | â | 141 | â | â | â | â |
| Loktin & Popova | 2017 | 0.73 | 0.23 | â | 192 | â | â | â | â |
| Joshi et al. | 2016 | 0.57 | 0.25 | â | 141 | â | 26 | â | â |
| Kharchenko et al. | 2016 | 0.57 | 0.25 | â | 141 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.57 | 0.25 | â | 141 | â | â | â | â |
| Piskunov et al. | 2008 | 0.55 | 0.25 | â | 141 | â | 48(1) | â | â |
| Piskunov et al. | 2007 | 0.55 | 0.25 | â | 141 | â | 12 | â | â |
| Kharchenko et al. | 2005 | 0.55 | 0.25 | â | 141 | â | â | â | â |
| Dias et al. | 2002 | 0.55 | 0.25 | â | 141 | 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.
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).
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.