ESO 313 03

(MWSC 1499)

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0.25 UTI
0.0
CN
0.04
Cdens
0.12
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members) 5.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.55 Moderately studied
  • Cdup 1.0 Unique

Overview

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ESO 313 03 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~6.72 kpc) differs significantly from the median photometric distance (~4.27 kpc).

Distant High extinction Intermediate age

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 127.915 -41.784 0.149 -3.174 3.504 94.606
Just et al. 2023 127.903 -41.784 – – – –
Cantat-Gaudin et al. 2020 127.907 -41.784 0.163 -3.189 3.492 –
Cantat-Gaudin & Anders 2020 127.907 -41.784 0.163 -3.189 3.492 –
Bica et al. 2019 127.925 -41.784 – – – –
Cantat-Gaudin et al. 2018 127.907 -41.784 0.163 -3.189 3.492 –
Kharchenko et al. 2016 127.903 -41.784 – – – –
Dias et al. 2014 127.921 -41.792 – -1.01 0.01 –
Kharchenko et al. 2013 127.908 -41.787 – -2.22 4.67 –
Dias et al. 2002 127.921 -41.792 – -2.22 4.67 –

💡 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] Bfr BSS
Just et al. 2023 – – – 398 – 339 – –
Cantat-Gaudin & Anders 2020 5.20 – – – – – – –
Cantat-Gaudin et al. 2018 5.20 – – – – – – –
Kharchenko et al. 2016 4.27 3.36 – 398 – – – –
Kharchenko et al. 2013 4.27 3.36 – 398 – – – –
Dias et al. 2002 3.05 2.85 – 708 – – – –

Visualization

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