ESO 493 03

(MWSC 1300)

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0.21 UTI
0.0
CN
0.01
Cdens
0.38
CC3
0.32
Clit
1.0
Cdup
Core radius and density 2.3 [pc], 0.06 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.01 Very loose
  • CC3 0.38 Low quality
  • Clit 0.32 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
ESO 493 03 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~6.58 kpc) differs significantly from the median photometric distance (~1.40 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– 114.916 -27.325 0.152 -1.456 2.143 89.856
Just et al. 2023 114.917 -27.293 – – – –
Dias et al. 2018 – – – -2.81 2.87 –
Dib et al. 2018 114.922 -27.295 – – – –
Loktin & Popova 2017 114.93 -27.293 – -2.878 1.754 20.77
Sampedro et al. 2017 114.938 -27.293 – – – –
Joshi et al. 2016 114.922 -27.295 – – – –
Kharchenko et al. 2016 114.917 -27.293 – – – –
Dias et al. 2014 114.938 -27.293 – -0.7 2.14 20.77
Kharchenko et al. 2013 114.922 -27.295 – -0.6 1.64 –
Piskunov et al. 2008 114.919 -27.287 – – – –
Kharchenko et al. 2005 114.93 -27.29 – 0.44 2.31 –
Dias et al. 2002 114.938 -27.293 – -0.72 2.15 20.77

💡 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– 1.4 0.32 – 243 – 170 – –
Just et al. 2023 – – – 243 – 101 – –
Dib et al. 2018 1.40 – – 243 – – – –
Loktin & Popova 2017 2.29 1.25 – 209 – – – –
Joshi et al. 2016 1.40 0.32 – 243 – 240 – –
Kharchenko et al. 2016 1.40 0.32 – 243 – – – –
Kharchenko et al. 2013 1.40 0.32 – 243 – – – –
Piskunov et al. 2008 1.40 0.32 – 398 – – – –
Kharchenko et al. 2005 1.40 0.32 – 398 – – – –
Dias et al. 2002 1.40 0.32 – 398 – – – –

Visualization

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