SAI 14

(MWSC 120)

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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

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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

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 21.492 62.623 0.221 -1.889 -1.086 -66.091
Hu & Soubiran 2025 21.517 62.627 – – – –
Almeida et al. 2025 21.517 62.629 – – – –
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 – – –
Hunt & Reffert 2023 21.491 62.617 0.212 -1.886 -1.097 -57.409
Just et al. 2023 21.506 62.61 – – – –
Dias et al. 2021 21.517 62.629 0.214 -1.906 -1.042 –
Cantat-Gaudin et al. 2020 21.504 62.624 0.23 -1.886 -1.058 –
SΓ‘nchez et al. 2020 21.5 62.626 – -1.865 -1.222 –
Cantat-Gaudin & Anders 2020 21.504 62.624 0.23 -1.886 -1.058 –
Bica et al. 2019 21.494 62.626 – – – –
Cantat-Gaudin et al. 2018 21.504 62.624 0.23 -1.886 -1.058 –
Loktin & Popova 2017 21.51 62.61 – 0.598 -0.707 –
Kharchenko et al. 2016 21.506 62.61 – – – –
Dias et al. 2014 21.5 62.626 – -1.18 -0.5 –
Kharchenko et al. 2013 21.517 62.613 – 2.24 -3.98 –
Kharchenko et al. 2012 21.517 62.613 – 2.24 -3.98 –
Glushkova et al. 2010 21.501 62.626 – – – –
Dias et al. 2002 21.5 62.626 – -1.18 -0.5 –

πŸ’‘ 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 – – – – -0.290* – – –
Almeida et al. 2025 4.95 3.20 – 659 – 644 – –
Hunt & Reffert 2024 – – – – – 1011* – –
Cavallo et al. 2024 4.43 3.54 – 589 -0.430 – – –
Hunt & Reffert 2023 3.87 3.27 2.08 540 – – – –
Just et al. 2023 – – – 2818 – 1239 – –
Dias et al. 2021 4.95 3.20 – 659 -0.012 – – –
Cantat-Gaudin et al. 2020 4.00 2.68 – 1349 – – – –
Cantat-Gaudin & Anders 2020 3.86 – – – – – – –
Cantat-Gaudin et al. 2018 3.86 – – – – – – –
Loktin & Popova 2017 4.77 2.56 – 741 – – – –
Kharchenko et al. 2016 5.09 2.58 – 2818 – – – –
Kharchenko et al. 2013 5.09 2.58 – 2818 – – – –
Kharchenko et al. 2012 5.09 2.58 – 2818 – – – –
Glushkova et al. 2010 6.46 1.71 – 1259 – – – –
Dias et al. 2002 6.46 1.71 – 1259 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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