ESO 021 06

(MWSC 2208)

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0.22 UTI
0.0
CN
0.1
Cdens
0.25
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 5.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.25 Low quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
ESO 021 06 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 massive, near-solar metallicity, old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.04 kpc) differs significantly from the median photometric distance (~2.47 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.

Relatively close Low extinction Massive Near-solar metallicity Old

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 213.701 -78.502 0.248 -8.956 -3.901 –
Just et al. 2023 213.945 -78.512 – – – –
Bica et al. 2019 213.959 -78.503 – – – –
Kharchenko et al. 2016 213.945 -78.512 – – – –
Dias et al. 2014 213.967 -78.503 – -3.1 -4.33 –
Kharchenko et al. 2013 213.966 -78.515 – -3.04 -5.85 –
Dias et al. 2002 213.967 -78.503 – -2.81 -3.68 –

💡 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
Just et al. 2023 – – – 3162 – 1714 – –
Kharchenko et al. 2016 2.47 0.32 – 3162 – – – –
Kharchenko et al. 2013 2.47 0.32 – 3162 – – – –
Dias et al. 2002 1.22 3.19 – 2239 -0.050 – – –

Visualization

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