SAI 109
(MWSC 1705)
0.91
UTI
0.79
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
2.0 [arcmin]
- 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
SAI 109 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster (see Parameters). It is very well-studied in the literature.
Very distant
Moderate extinction
Massive
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 145.913 | -50.797 | 0.126 | -4.436 | 3.725 | 82.417 |
| Hu & Soubiran | 2025 | 145.903 | -50.803 | â | â | â | â |
| Almeida et al. | 2025 | 145.893 | -50.802 | â | â | â | â |
| Hunt & Reffert | 2024 | 145.922 | -50.795 | 0.135 | -4.424 | 3.685 | 80.402 |
| Cavallo et al. | 2024 | 145.903 | -50.803 | 0.133 | â | â | â |
| Hunt & Reffert | 2023 | 145.922 | -50.795 | 0.135 | -4.424 | 3.685 | 80.402 |
| Just et al. | 2023 | 145.9 | -50.78 | â | â | â | â |
| Dias et al. | 2021 | 145.893 | -50.802 | 0.07 | -4.43 | 3.778 | â |
| Cantat-Gaudin et al. | 2020 | 145.902 | -50.797 | 0.095 | -4.378 | 3.825 | â |
| Cantat-Gaudin & Anders | 2020 | 145.902 | -50.797 | 0.095 | -4.378 | 3.825 | â |
| Soubiran et al. | 2018 | 145.902 | -50.797 | â | â | â | 82.33 |
| Bica et al. | 2019 | 145.892 | -50.797 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 145.902 | -50.797 | 0.095 | -4.378 | 3.825 | â |
| Kharchenko et al. | 2016 | 145.9 | -50.78 | â | â | â | â |
| Dias et al. | 2014 | 145.892 | -50.792 | â | -6.79 | 3.33 | â |
| Kharchenko et al. | 2013 | 145.905 | -50.783 | â | -6.5 | 7.12 | â |
| Glushkova et al. | 2010 | 145.893 | -50.792 | â | â | â | â |
| Dias et al. | 2002 | 145.892 | -50.792 | â | -6.79 | 3.33 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.210* | â | â | â |
| Almeida et al. | 2025 | 7.55 | 2.28 | â | 918 | â | 1490 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1866* | â | â |
| Cavallo et al. | 2024 | 5.97 | 2.04 | â | 955 | -0.050 | â | â | â |
| Hunt & Reffert | 2023 | 6.57 | 2.29 | 1.94 | 767 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1000 | â | 885 | â | â |
| Dias et al. | 2021 | 7.55 | 2.28 | â | 918 | -0.173 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 7.14 | 1.78 | â | 1047 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 8.07 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 8.07 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 8.07 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 5.25 | 1.94 | â | 1000 | â | â | â | â |
| Kharchenko et al. | 2013 | 5.25 | 1.94 | â | 1000 | â | â | â | â |
| Glushkova et al. | 2010 | 7.69 | 0.71 | â | 1585 | â | â | â | â |
| Dias et al. | 2002 | 7.69 | 0.71 | â | 1585 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.