ESO 435 33

(MWSC 1753)

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0.11 UTI
0.0
CN
0.02
Cdens
0.12
CC3
0.19
Clit
1.0
Cdup
Core radius and density 7.6 [pc], 0.08 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.19 Rarely studied
  • Cdup 1.0 Unique

Overview

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ESO 435 33 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, well above the mid-plane, affected by low extinction. It is catalogued as a low-mass, old cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~2.63 kpc) differs significantly from the median photometric distance (~1.18 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– 151.069 -32.031 0.381 -8.044 2.942 20.095
Just et al. 2023 150.968 -32.046 – – – –
Bica et al. 2019 150.965 -32.057 – – – –
Joshi et al. 2016 150.975 -32.05 – – – –
Kharchenko et al. 2016 150.968 -32.046 – – – –
Kharchenko et al. 2013 150.975 -32.05 – -2.32 2.16 –
Bukowiecki et al. 2011 150.971 -32.048 – – – –
Dias et al. 2002 150.975 -32.053 – -5.17 -0.5 –

💡 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– 1.18 0.85 – 1122 – 28 – –
Just et al. 2023 – – – 1122 – 14 – –
Joshi et al. 2016 1.18 0.85 – 1122 – – – –
Kharchenko et al. 2016 1.18 0.85 – 1122 – – – –
Kharchenko et al. 2013 1.18 0.85 – 1122 – – – –
Bukowiecki et al. 2012 – – – – – 43 – –
Bukowiecki et al. 2011 2.89(1) 3.19 – 141 – – – –
Dias et al. 2002 2.86 3.28 – 141 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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