NGC 6588
(MWSC 2895)
0.11
UTI
0.25
CN
0.03
Cdens
0.12
CC3
0.06
Clit
1.0
Cdup
Nm (P>50%)
25
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
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).
â 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
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 275.092 | -63.877 | 0.31 | -1.478 | -3.709 | â |
| Bica et al. | 2019 | 275.146 | -63.803 | â | â | â | â |
| Sampedro et al. | 2017 | 275.137 | -63.808 | â | â | â | â |
| Tadross | 2014 | 275.137 | -63.808 | â | â | â | â |
| Dias et al. | 2002 | 275.137 | -63.808 | â | -2.06 | -8.25 | â |
đĄ 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 | 99999â | 1.635 | 0.285 | â | 3034 | -0.240 | â | â | â |
| Tadross | 2014 | 0.96 | 0.32 | â | 1600 | â | â | â | â |
| Dias et al. | 2002 | 2.31 | 0.25 | â | 4467 | -0.240 | â | â | â |
MOCA

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).