SAI 14
(MWSC 120)
0.85
UTI
0.76
CN
1.0
Cdens
0.5
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
2.2 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
SAI 14 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is very well-studied in the literature.
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 | β | 21.492 | 62.623 | 0.221 | -1.889 | -1.086 | -66.091 |
| Hu & Soubiran | 2025 | 21.517 | 62.627 | β | β | β | β |
| Almeida et al. | 2025 | 21.517 | 62.629 | β | β | β | β |
| Hunt & Reffert | 2024 | 21.491 | 62.617 | 0.212 | -1.886 | -1.097 | -57.409 |
| Cavallo et al. | 2024 | 21.517 | 62.627 | 0.211 | β | β | β |
| Hunt & Reffert | 2023 | 21.491 | 62.617 | 0.212 | -1.886 | -1.097 | -57.409 |
| Just et al. | 2023 | 21.506 | 62.61 | β | β | β | β |
| Dias et al. | 2021 | 21.517 | 62.629 | 0.214 | -1.906 | -1.042 | β |
| Cantat-Gaudin et al. | 2020 | 21.504 | 62.624 | 0.23 | -1.886 | -1.058 | β |
| SΓ‘nchez et al. | 2020 | 21.5 | 62.626 | β | -1.865 | -1.222 | β |
| Cantat-Gaudin & Anders | 2020 | 21.504 | 62.624 | 0.23 | -1.886 | -1.058 | β |
| Bica et al. | 2019 | 21.494 | 62.626 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 21.504 | 62.624 | 0.23 | -1.886 | -1.058 | β |
| Loktin & Popova | 2017 | 21.51 | 62.61 | β | 0.598 | -0.707 | β |
| Kharchenko et al. | 2016 | 21.506 | 62.61 | β | β | β | β |
| Dias et al. | 2014 | 21.5 | 62.626 | β | -1.18 | -0.5 | β |
| Kharchenko et al. | 2013 | 21.517 | 62.613 | β | 2.24 | -3.98 | β |
| Kharchenko et al. | 2012 | 21.517 | 62.613 | β | 2.24 | -3.98 | β |
| Glushkova et al. | 2010 | 21.501 | 62.626 | β | β | β | β |
| Dias et al. | 2002 | 21.5 | 62.626 | β | -1.18 | -0.5 | β |
π‘ 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 | β | β | β | β | -0.290* | β | β | β |
| Almeida et al. | 2025 | 4.95 | 3.20 | β | 659 | β | 644 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1011* | β | β |
| Cavallo et al. | 2024 | 4.43 | 3.54 | β | 589 | -0.430 | β | β | β |
| Hunt & Reffert | 2023 | 3.87 | 3.27 | 2.08 | 540 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 2818 | β | 1239 | β | β |
| Dias et al. | 2021 | 4.95 | 3.20 | β | 659 | -0.012 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 4.00 | 2.68 | β | 1349 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.86 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.86 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 4.77 | 2.56 | β | 741 | β | β | β | β |
| Kharchenko et al. | 2016 | 5.09 | 2.58 | β | 2818 | β | β | β | β |
| Kharchenko et al. | 2013 | 5.09 | 2.58 | β | 2818 | β | β | β | β |
| Kharchenko et al. | 2012 | 5.09 | 2.58 | β | 2818 | β | β | β | β |
| Glushkova et al. | 2010 | 6.46 | 1.71 | β | 1259 | β | β | β | β |
| Dias et al. | 2002 | 6.46 | 1.71 | β | 1259 | β | β | β | β |
(*): 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. Silver sample.
Cavallo et al. (2024)
Gold sample.