NGC 6588

(MWSC 2895)

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0.11 UTI
0.25
CN
0.03
Cdens
0.12
CC3
0.06
Clit
1.0
Cdup
Core radius and density 5.2 [pc], 0.2 [pc-2]
  • CN 0.25 Poorly populated
  • Cdens 0.03 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
NGC 6588 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, well below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~3.23 kpc) differs significantly from the median photometric distance (~1.64 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.

Dias et al. (2022)
Likely not a real open cluster.

Cantat-Gaudin & Anders (2020)
Non-existent in early catalogues; literature distances and ages are highly discrepant, reflecting uncertain nature. More details in Appendix A of the article.

Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 275.092 -63.877 0.31 -1.478 -3.709 –
Bica et al. 2019 275.146 -63.803 – – – –
Sampedro et al. 2017 275.137 -63.808 – – – –
Tadross 2014 275.137 -63.808 – – – –
Dias et al. 2002 275.137 -63.808 – -2.06 -8.25 –

💡 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– 1.635 0.285 – 3034 -0.240 – – –
Tadross 2014 0.96 0.32 – 1600 – – – –
Dias et al. 2002 2.31 0.25 – 4467 -0.240 – – –

Visualization

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