ESO 561 05

(MWSC 1402)

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0.16 UTI
0.0
CN
0.03
Cdens
0.12
CC3
0.32
Clit
1.0
Cdup
Core radius and density 2.6 [pc], 0.1 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.03 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.32 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
ESO 561 05 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.23 kpc) differs significantly from the median photometric distance (~2.77 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

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 119.824 -22.717 0.236 -2.366 1.888 89.143
Just et al. 2023 119.823 -22.687 – – – –
Bica et al. 2019 119.821 -22.689 – – – –
Dias et al. 2018 – – – -2.92 1.66 –
Dib et al. 2018 119.829 -22.69 – – – –
Loktin & Popova 2017 119.835 -22.692 – -0.334 3.581 –
Sampedro et al. 2017 119.829 -22.692 – -3.63 3.14 –
Kharchenko et al. 2016 119.823 -22.687 – – – –
Dias et al. 2014 119.829 -22.692 – -3.58 3.85 –
Kharchenko et al. 2013 119.829 -22.69 – 1.11 3.79 –
Bukowiecki et al. 2011 119.825 -22.696 – – – –
Dias et al. 2002 119.829 -22.692 – -3.58 3.85 –

💡 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– 2.77 0.46 – 1000 – 312 – –
Just et al. 2023 – – – 1000 – 265 – –
Dib et al. 2018 1.86 – – 1000 – – – –
Loktin & Popova 2017 4.24 0.00 – 832 – – – –
Kharchenko et al. 2016 1.86 0.46 – 1000 – – – –
Kharchenko et al. 2013 1.86 0.46 – 1000 – – – –
Bukowiecki et al. 2012 – – – – – 358 – –
Bukowiecki et al. 2011 3.69(1) 1.14 – 224 – – – –
Dias et al. 2002 3.68 1.17 – 224 – – – –

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

Visualization

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