MWSC 4463

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0.08 UTI
0.0
CN
0.04
Cdens
0.12
CC3
0.13
Clit
1.0
Cdup
Core radius and density 1.9 [pc], 0.2 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.13 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
MWSC 4463 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~2.39 kpc) differs significantly from the median photometric distance (~1.41 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– 284.741 -64.238 0.419 -2.265 -2.115 –
Just et al. 2023 284.716 -64.266 – – – –
Bica et al. 2019 284.734 -64.269 – – – –
Dib et al. 2018 284.73 -64.265 – – – –
Joshi et al. 2016 284.73 -64.265 – – – –
Kharchenko et al. 2016 284.716 -64.266 – – – –
Scholz et al. 2015 284.73 -64.265 – 0.94 -5.41 –

💡 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– 1.41 1.09 – 1413 – 142 – –
Just et al. 2023 – – – 1413 – 142 – –
Dib et al. 2018 1.41 – – 1413 – – – –
Joshi et al. 2016 1.41 1.09 – 1413 – – – –
Kharchenko et al. 2016 1.41 1.09 – 1413 – – – –
Scholz et al. 2015 1.41 1.09 – 1413 – – – –

Visualization

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