NGC 2189

(MWSC 788)

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0.10 UTI
0.0
CN
0.05
Cdens
0.12
CC3
0.16
Clit
1.0
Cdup
Core radius and density 2.8 [pc], 0.2 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.05 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.16 Rarely studied
  • Cdup 1.0 Unique

Overview

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NGC 2189 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~2.97 kpc) differs significantly from the median photometric distance (~1.47 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.

Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010).

Dias et al. (2002)
Not found (Archinal, B. A. & Hynes, S. J. 2003); cat V3.5 (Jan 2016)

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 93.067 1.083 0.336 -0.159 -1.942 31.802
Just et al. 2023 93.023 1.056 – – – –
Bica et al. 2019 93.08 1.136 – – – –
Dib et al. 2018 93.03 1.055 – – – –
Joshi et al. 2016 93.03 1.055 – – – –
Kharchenko et al. 2016 93.023 1.056 – – – –
Tadross 2014 93.037 1.065 – – – –
Kharchenko et al. 2013 93.03 1.055 – 1.88 -2.16 –

💡 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– 1.47 0.66 – 1496 – 62 – –
Just et al. 2023 – – – 1496 – 62 – –
Dib et al. 2018 1.47 – – 1496 – – – –
Joshi et al. 2016 1.47 0.66 – 1496 – – – –
Kharchenko et al. 2016 1.47 0.66 – 1496 – – – –
Tadross 2014 1.87 1.23 – 800 – – – –
Kharchenko et al. 2013 1.47 0.66 – 1496 – – – –

Visualization

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