ESO 436 02

(MWSC 1780)

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0.13 UTI
0.0
CN
0.03
Cdens
0.25
CC3
0.19
Clit
1.0
Cdup
Core radius and density 3.2 [pc], 0.1 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.03 Very loose
  • CC3 0.25 Low quality
  • Clit 0.19 Rarely studied
  • Cdup 1.0 Unique

Overview

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ESO 436 02 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, well above 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 (~2.76 kpc) differs significantly from the median photometric distance (~1.37 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– 153.466 -29.153 0.362 -6.324 1.943 46.542
Just et al. 2023 153.482 -29.165 – – – –
Sampedro et al. 2017 153.512 -29.19 – – – –
Joshi et al. 2016 153.489 -29.168 – – – –
Kharchenko et al. 2016 153.482 -29.165 – – – –
Kharchenko et al. 2013 153.489 -29.168 – -5.45 3.05 –
Bukowiecki et al. 2011 153.492 -29.186 – – – –
Dias et al. 2002 153.512 -29.19 – -20.48 -1.44 –

💡 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– 1.37 0.16 – 1259 – 120 – –
Just et al. 2023 – – – 1259 – 158 – –
Joshi et al. 2016 1.37 0.16 – 1259 – – – –
Kharchenko et al. 2016 1.37 0.16 – 1259 – – – –
Kharchenko et al. 2013 1.37 0.16 – 1259 – – – –
Bukowiecki et al. 2012 – – – – – 81 – –
Bukowiecki et al. 2011 2.17(1) 2.52 – 178 – – – –
Dias et al. 2002 2.15 2.62 – 178 – – – –

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

Visualization

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