Alessi Teutsch 9
(ASCC 10; MWSC 275; AT 9)
0.93
UTI
0.72
CN
0.95
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
4.8 [N/pc2]
- CN 0.72 Moderately populated
- Cdens 0.95 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Alessi Teutsch 9 is a moderately populated, 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 and metallicity 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 | 51.827 | 34.88 | 1.506 | -1.78 | -1.426 | -18.531 |
| Li et al. | 2025 | 51.87 | 34.981 | 1.459 | -1.737 | -1.368 | â |
| Almeida et al. | 2025 | 51.874 | 35.011 | â | â | â | â |
| Alfonso et al. | 2024 | 51.784 | 34.847 | 1.45 | -1.816 | -1.47 | â |
| Zhang et al. | 2024 | 51.863 | 34.886 | â | â | â | â |
| Hunt & Reffert | 2024 | 51.863 | 34.886 | 1.507 | -1.853 | -1.359 | -16.806 |
| Cavallo et al. | 2024 | 51.033 | 35.538 | 1.51 | â | â | â |
| Hunt & Reffert | 2023 | 51.863 | 34.886 | 1.507 | -1.853 | -1.359 | -16.806 |
| Almeida et al. | 2023 | 51.906 | 35.011 | â | â | â | â |
| Just et al. | 2023 | 51.756 | 35.028 | â | â | â | â |
| He et al. | 2022 | 51.858 | 34.897 | 1.518 | -1.779 | -1.43 | â |
| Tarricq et al. | 2022 | 51.807 | 34.945 | 1.491 | -1.839 | -1.396 | â |
| Dias et al. | 2021 | 51.874 | 35.011 | 1.465 | -1.704 | -1.348 | -10.87 |
| Cantat-Gaudin et al. | 2020 | 51.87 | 34.981 | 1.459 | -1.737 | -1.368 | â |
| Cantat-Gaudin & Anders | 2020 | 51.87 | 34.981 | 1.459 | -1.737 | -1.368 | â |
| Bossini et al. | 2019 | 51.87 | 34.981 | â | â | â | â |
| Soubiran et al. | 2018 | 51.87 | 34.981 | â | â | â | -15.67 |
| Bica et al. | 2019 | 51.864 | 34.947 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 51.87 | 34.981 | 1.459 | -1.737 | -1.368 | â |
| Kharchenko et al. | 2016 | 51.756 | 35.028 | â | â | â | â |
| Dias et al. | 2014 | 51.862 | 34.953 | â | 1.17 | -2.05 | â |
| Kharchenko et al. | 2013 | 51.765 | 35.03 | â | -2.9 | -1.6 | â |
| Kharchenko et al. | 2012 | 51.765 | 35.03 | â | -2.9 | -1.6 | â |
| Piskunov et al. | 2008 | 51.739 | 35.034 | â | â | â | â |
| Kharchenko et al. | 2005 | 51.75 | 35.04 | â | -3.08 | -1.01 | â |
| Dias et al. | 2002 | 51.862 | 34.953 | â | -3.08 | -1.01 | 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 | 0.67 | 0.63 | 1.09 | 376 | 0.004 | 180 | 0.45 | â |
| Li et al. | 2025 | 0.63 | 0.69 | â | 385 | -0.041 | â | â | â |
| Almeida et al. | 2025 | 0.64 | 0.82 | â | 151 | â | 146 | â | â |
| Alfonso et al. | 2024 | 0.66 | 0.63 | â | 368 | 0.109 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.016(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 153(1) | â | â |
| Cavallo et al. | 2024 | 0.67 | 0.89 | â | 95 | 0.300 | â | â | â |
| Hunt & Reffert | 2023 | 0.63 | 0.70 | 1.09 | 78 | â | â | â | â |
| Almeida et al. | 2023 | 0.64 | 0.79 | â | 196 | 0.004 | 229(1) | 0.45 | â |
| Just et al. | 2023 | â | â | â | 521 | â | 207 | â | â |
| He et al. | 2022 | â | 0.75 | â | 79 | â | â | â | â |
| Tarricq et al. | 2022 | 0.65 | â | â | 263 | â | â | â | â |
| Dias et al. | 2021 | 0.64 | 0.82 | â | 151 | 0.109 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.66 | 0.63 | â | 263 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.67 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 0.61 | 0.44 | â | 397 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.67 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.67 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 0.70 | 0.31 | â | 521 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.70 | 0.31 | â | 521 | â | â | â | â |
| Kharchenko et al. | 2012 | 0.70 | 0.31 | â | 521 | â | â | â | â |
| Piskunov et al. | 2008 | 0.70 | 0.31 | â | 447 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.70 | 0.31 | â | 447 | â | â | â | â |
| Dias et al. | 2002 | 0.70 | 0.31 | â | 447 | 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.
Cavallo et al. (2024)
Gold sample.