NGC 6737
(MWSC 3042; ESO 592 08)
0.17
UTI
0.26
CN
0.03
Cdens
0.12
CC3
0.23
Clit
1.0
Cdup
Nm (P>50%)
26
Core radius and density
2.5 [pc], 0.2 [pc-2]
- CN 0.26 Poorly populated
- Cdens 0.03 Very loose
- CC3 0.12 Very low quality
- Clit 0.23 Rarely studied
- Cdup 1.0 Unique
Overview
NGC 6737 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 moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature.
(*): The parallax distance estimate (~3.77 kpc) differs significantly from the median photometric distance (~2.08 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 | 285.588 | -18.578 | 0.265 | -6.521 | -4.972 | 45.455 |
| Just et al. | 2023 | 285.575 | -18.535 | â | â | â | â |
| Bica et al. | 2019 | 285.548 | -18.549 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -1.02 | -3.2 | â |
| Loktin & Popova | 2017 | 285.585 | -18.55 | â | 1.728 | -5.899 | â |
| Sampedro et al. | 2017 | 285.583 | -18.55 | â | -0.69 | -2.1 | â |
| Kharchenko et al. | 2016 | 285.575 | -18.535 | â | â | â | â |
| Tadross | 2014 | 285.583 | -18.55 | â | â | â | â |
| Dias et al. | 2014 | 285.583 | -18.55 | â | -0.97 | -1.75 | â |
| Kharchenko et al. | 2013 | 285.583 | -18.533 | â | -1.01 | -4.0 | 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 | 2.08 | 2.45 | â | 794 | â | 276 | â | â |
| Just et al. | 2023 | â | â | â | 794 | â | 276 | â | â |
| Loktin & Popova | 2017 | 2.66 | 0.91 | â | 1778 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.04 | 2.50 | â | 794 | â | â | â | â |
| Tadross | 2014 | 2.12 | 2.40 | â | 500 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.04 | 2.50 | â | 794 | â | â | â | â |
MOCA
