Alessi Teutsch 3
(ASCC 42; MWSC 1373; AT 3; Alessi 30)
0.91
UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.9
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 0.9 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, but with a large variance across recent sources for the age 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 | 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 |
| Richer et al. | 2021 | 118.261 | -53.058 | 1.39 | -5.367 | 8.892 | 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 |
| Dib et al. | 2018 | 118.14 | -52.995 | â | â | â | â |
| Loktin & Popova | 2017 | 118.26 | -53.044 | â | -1.918 | 8.792 | 15.0 |
| Sampedro et al. | 2017 | 118.254 | -53.045 | -4.42 | 5.63 | â | â |
| Joshi et al. | 2016 | 118.14 | -52.995 | â | â | â | â |
| 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 | 0.53 | 1.09 | 141 | 0.011 | 222 | 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 |
| Richer et al. | 2021 | â | 0.53 | â | 400 | 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 |
| Kounkel et al. | 2020 | 0.69 | 0.68 | â | 83 | 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 |
| Dib et al. | 2018 | 0.79 | â | â | 141 | â | â | â | â |
| Loktin & Popova | 2017 | 0.88 | 0.75 | â | 618 | â | â | â | â |
| Joshi et al. | 2016 | 0.79 | 0.53 | â | 141 | â | 617 | â | â |
| Kharchenko et al. | 2016 | 0.79 | 0.53 | â | 141 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.79 | 0.53 | â | 141 | â | â | â | â |
| Piskunov et al. | 2008 | 0.80 | 0.32 | â | 372 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.80 | 0.32 | â | 372 | â | â | â | â |
| Dias et al. | 2002 | 0.80 | 0.32 | â | 372 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P35, along with HSC_2154.
Almeida et al. (2025)
Mass determination: intermediate 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 8.4, 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.