SAI 122

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0.64 UTI
0.84
CN
1.0
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.84 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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SAI 122 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near 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 moderate 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 – 225.071 -58.802 0.294 -3.161 -2.389 -48.404
Hunt & Reffert 2024 225.069 -58.809 0.297 -3.16 -2.393 -36.807
Cavallo et al. 2024 225.094 -58.803 0.301 – – –
Hunt & Reffert 2023 225.069 -58.809 0.297 -3.16 -2.393 -36.807
Bica et al. 2019 225.028 -58.804 – – – –
Glushkova et al. 2010 225.016 -58.804 – – – –

💡 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 – – – – – 5339* – –
Cavallo et al. 2024 3.47 5.94 – 40 0.330 – – –
Hunt & Reffert 2023 2.67 5.52 2.94 834 – – – –
Glushkova et al. 2010 1.67 7.01 – 178 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2263 42.5 225.07 -58.8 0.31 -3.17 -2.42 -48.68 0.0

💡 Note: The % column shows the percentage of members that SAI 122 shares with each listed object.

Visualization

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