SAI 123

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0.69 UTI
0.8
CN
1.0
Cdens
1.0
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 2.1 [arcmin]
  • CN 0.8 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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SAI 123 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by very high extinction. It is catalogued as a very massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close Very high extinction Very massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 242.082 -50.521 0.298 -2.79 -3.643 -44.614
Hunt & Reffert 2024 242.088 -50.522 0.3 -2.798 -3.631 -39.348
Cavallo et al. 2024 242.078 -50.515 0.292 – – –
Hunt & Reffert 2023 242.088 -50.522 0.3 -2.798 -3.631 -39.348
Bica et al. 2019 242.072 -50.54 – – – –
Glushkova et al. 2010 242.072 -50.535 – – – –

💡 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
Hunt & Reffert 2024 – – – – – 6118* – –
Cavallo et al. 2024 3.50 5.83 – 35 0.360 – – –
Hunt & Reffert 2023 2.96 6.32 2.26 352 – – – –
Glushkova et al. 2010 1.86 4.19 – 1585 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1546 80.8 242.08 -50.52 0.29 -2.79 -3.64 -44.87 0.0

💡 Note: The % column shows the percentage of members that SAI 123 shares with each listed object.

Visualization

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