ASCC 82

(MWSC 2320)

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0.24 UTI
0.0
CN
0.04
Cdens
0.25
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad) 0.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.25 Low quality
  • Clit 0.45 Poorly studied
  • Cdup 1.0 Unique

Overview

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

(*): The parallax distance estimate (~4.23 kpc) differs significantly from the median photometric distance (~0.80 kpc).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 236.868 -64.426 0.236 -3.093 -3.746 -46.862
Just et al. 2023 236.746 -64.41 – – – –
Bica et al. 2019 236.841 -64.412 – – – –
Kharchenko et al. 2016 236.746 -64.41 – – – –
Dias et al. 2014 236.85 -64.41 – -4.52 -4.31 –
Kharchenko et al. 2013 236.76 -64.412 – -2.34 -5.16 –
Piskunov et al. 2008 236.84 -64.412 – – – –
Kharchenko et al. 2005 236.85 -64.41 – -2.96 -5.23 –
Dias et al. 2002 236.85 -64.41 – -4.52 -4.31 –

💡 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– 0.8 0.0 – 433 – 22 – –
Just et al. 2023 – – – 398 – 22 – –
Kharchenko et al. 2016 0.80 0.00 – 398 – – – –
Kharchenko et al. 2013 0.80 0.00 – 398 – – – –
Piskunov et al. 2008 0.80 0.00 – 468 – – – –
Kharchenko et al. 2005 0.80 0.00 – 468 – – – –
Dias et al. 2002 0.80 0.00 – 468 – – – –

Visualization

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