Alessi Teutsch 5
(ASCC 118; AT 5; Alessi 27; MWSC 3589)
0.91
UTI
0.79
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
23.8 [N/pc2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Alessi Teutsch 5 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is very well-studied in the literature.
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 332.152 | 61.103 | 1.115 | -1.901 | -3.272 | -22.755 |
| Almeida et al. | 2025 | 332.274 | 61.096 | â | â | â | â |
| Alfonso et al. | 2024 | 333.452 | 61.239 | 1.091 | -1.391 | -3.114 | â |
| Hunt & Reffert | 2024 | 332.043 | 61.052 | 1.126 | -1.88 | -3.329 | -22.773 |
| Celli et al. | 2024 | 332.218 | 61.103 | â | â | â | â |
| Cavallo et al. | 2024 | 332.085 | 61.065 | 1.123 | â | â | â |
| Hunt & Reffert | 2023 | 332.043 | 61.052 | 1.126 | -1.88 | -3.329 | -22.773 |
| He et al. | 2022 | 333.275 | 61.36 | 1.114 | -1.43 | -3.086 | â |
| Dias et al. | 2021 | 332.274 | 61.096 | 1.127 | -1.943 | -3.205 | â |
| Cantat-Gaudin et al. | 2020 | 332.218 | 61.103 | 1.111 | -1.895 | -3.207 | â |
| Cantat-Gaudin & Anders | 2020 | 332.218 | 61.103 | 1.111 | -1.895 | -3.207 | â |
| Dias et al. | 2019 | 332.217 | 61.103 | 1.111 | -1.895 | -3.207 | -5.04 |
| Soubiran et al. | 2018 | 332.218 | 61.103 | â | â | â | -21.04 |
| Bica et al. | 2019 | 332.108 | 61.03 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 332.218 | 61.103 | 1.111 | -1.895 | -3.207 | â |
| Loktin & Popova | 2017 | 332.115 | 61.028 | â | -1.017 | -0.935 | -42.0 |
| Dias et al. | 2014 | 332.112 | 61.028 | â | -0.96 | -2.81 | â |
| Gozha et al. | 2012 | 332.112 | 61.028 | â | â | â | â |
| Piskunov et al. | 2008 | 332.087 | 61.096 | â | â | â | â |
| Kharchenko et al. | 2007 | 332.1 | 61.1 | â | 0.21 | â | -42.0 |
| Kharchenko et al. | 2005 | 332.1 | 61.1 | â | -2.19 | -4.03 | -42.0 |
| Dias et al. | 2002 | 332.113 | 61.028 | â | -0.96 | -2.81 | -42.0 |
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 | 0.88 | 1.045 | 1.29 | 11 | -0.141 | 269 | â | â |
| Almeida et al. | 2025 | 0.87 | 1.25 | â | 12 | â | 453 | â | â |
| Alfonso et al. | 2024 | 0.86 | 1.02 | â | 14 | -0.050 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 222(1) | â | â |
| Celli et al. | 2024 | â | â | â | 19 | â | 316 | â | â |
| Cavallo et al. | 2024 | 0.89 | 1.41 | â | 5 | -0.230 | â | â | â |
| Hunt & Reffert | 2023 | 0.87 | 0.91 | 1.29 | 6 | â | â | â | â |
| He et al. | 2022 | â | 1.10 | â | 2 | â | â | â | â |
| Dias et al. | 2021 | 0.87 | 1.25 | â | 12 | -0.053 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.91 | 1.02 | â | 19 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.88 | â | â | â | â | â | â | â |
| Dias et al. | 2019 | 0.80 | 1.24 | â | 13 | -0.930 | â | â | â |
| Soubiran et al. | 2018 | 0.88 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.88 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.08 | 1.07 | â | 26 | â | â | â | â |
| Gozha et al. | 2012 | 0.90 | â | â | 10 | â | 95 | â | â |
| Piskunov et al. | 2008 | 0.90 | 0.93 | â | 10 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.90 | 0.93 | â | 10 | â | â | â | â |
| Dias et al. | 2002 | 0.90 | 0.93 | â | 10 | 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: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.