SAI 82

(MWSC 1366)

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0.17 UTI
0.27
CN
0.01
Cdens
0.12
CC3
0.23
Clit
1.0
Cdup
Core radius and density 3.1 [pc], 0.03 [pc-2]
  • CN 0.27 Poorly populated
  • Cdens 0.01 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.23 Rarely studied
  • Cdup 1.0 Unique

Overview

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SAI 82 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~3.13 kpc) differs significantly from the median photometric distance (~1.44 kpc).

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 118.059 -33.089 0.32 -3.732 4.509 24.488
Just et al. 2023 118.051 -33.037 – – – –
Bica et al. 2019 118.06 -33.044 – – – –
Dib et al. 2018 118.056 -33.04 – – – –
Sampedro et al. 2017 118.058 -33.041 – – – –
Joshi et al. 2016 118.056 -33.04 – – – –
Kharchenko et al. 2016 118.051 -33.037 – – – –
Kharchenko et al. 2013 118.056 -33.04 – -3.58 9.46 –
Glushkova et al. 2010 118.06 -33.041 – – – –
Dias et al. 2002 118.058 -33.041 – 0.42 3.74 –

💡 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] Bfrac BSS
UCC 99999– 1.44 2.1 – 447 – 25 – –
Just et al. 2023 – – – 447 – 25 – –
Dib et al. 2018 1.44 – – 447 – – – –
Joshi et al. 2016 1.44 2.10 – 447 – – – –
Kharchenko et al. 2016 1.44 2.10 – 447 – – – –
Kharchenko et al. 2013 1.44 2.10 – 447 – – – –
Glushkova et al. 2010 1.15 1.23 – 447 – – – –
Dias et al. 2002 1.15 1.23 – 447 – – – –

Visualization

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