NGC 5043

(MWSC 2099; ESO 132 02)

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0.22 UTI
0.0
CN
0.07
Cdens
0.12
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad) 0.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.07 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.45 Poorly studied
  • Cdup 1.0 Unique

Overview

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NGC 5043 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 a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.80 kpc) differs significantly from the median photometric distance (~0.97 kpc).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 199.036 -60.071 0.264 -9.373 -1.395 28.324
Just et al. 2023 199.009 -60.062 – – – –
Bica et al. 2019 199.034 -60.084 – – – –
Kharchenko et al. 2016 199.009 -60.062 – – – –
Dias et al. 2014 199.037 -60.073 – -7.6 -1.48 –
Kharchenko et al. 2013 199.02 -60.065 – -11.03 -1.07 –
Piskunov et al. 2008 199.03 -60.064 – – – –
Kharchenko et al. 2005 199.03 -60.07 – -10.6 -0.86 –
Dias et al. 2002 199.037 -60.073 – -7.72 -1.52 –

💡 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– 0.97 0.46 – 508 – 48 – –
Just et al. 2023 – – – 398 – 48 – –
Kharchenko et al. 2016 0.86 0.26 – 398 – – – –
Kharchenko et al. 2013 0.86 0.26 – 398 – – – –
Piskunov et al. 2008 0.97 0.46 – 617 – – – –
Kharchenko et al. 2005 0.97 0.46 – 617 – – – –
Dias et al. 2002 0.97 0.46 – 617 – – – –

Visualization

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