ESO 309 03

(MWSC 998)

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0.15 UTI
0.0
CN
0.02
Cdens
0.25
CC3
0.23
Clit
1.0
Cdup
Stellar density (N50/rad) 0.1 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.25 Low quality
  • Clit 0.23 Rarely studied
  • Cdup 1.0 Unique

Overview

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ESO 309 03 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~5.91 kpc) differs significantly from the median photometric distance (~2.06 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– 102.646 -42.404 0.169 -0.765 2.669 68.393
Just et al. 2023 102.659 -42.381 – – – –
Bica et al. 2019 102.671 -42.38 – – – –
Loktin & Popova 2017 102.66 -42.39 – -0.019 0.452 –
Sampedro et al. 2017 102.662 -42.39 16.85 -40.55 – –
Kharchenko et al. 2016 102.659 -42.381 – – – –
Kharchenko et al. 2013 102.663 -42.383 – 0.07 -0.35 –
Bukowiecki et al. 2011 102.658 -42.383 – – – –
Dias et al. 2002 102.662 -42.39 – -0.2 1.93 –

💡 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– 2.06 1.31 – 876 – 84 – –
Just et al. 2023 – – – 1122 – 88 – –
Loktin & Popova 2017 2.81 0.42 – 1 – – – –
Kharchenko et al. 2016 2.06 1.31 – 1122 – – – –
Kharchenko et al. 2013 2.06 1.31 – 1122 – – – –
Bukowiecki et al. 2012 – – – – – 79 – –
Bukowiecki et al. 2011 1.76(1) 1.48 – 631 – – – –
Dias et al. 2002 1.75 1.51 – 631 – – – –

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

Visualization

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