NGC 6334
0.43
UTI
0.56
CN
0.28
Cdens
0.75
CC3
0.29
Clit
1.0
Cdup
Nm (P>50%)
62
Core radius and density
1.1 [pc], 1.4 [pc-2]
- CN 0.56 Moderately populated
- Cdens 0.28 Loose
- CC3 0.75 High quality
- Clit 0.29 Poorly studied
- Cdup 1.0 Unique
Overview
NGC 6334 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a moderate percentage of members with 8 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 260.044 | -36.052 | 0.561 | 0.146 | -1.747 | -29.568 |
| Hunt & Reffert | 2024 | 259.951 | -36.085 | 0.565 | 0.132 | -1.781 | 0.778 |
| Cavallo et al. | 2024 | 260.043 | -35.956 | 0.565 | â | â | â |
| Hunt & Reffert | 2023 | 259.951 | -36.085 | 0.565 | 0.132 | -1.781 | 0.778 |
| Dias et al. | 2018 | â | â | â | -0.71 | -3.47 | â |
| Dib et al. | 2018 | 260.212 | -36.115 | â | â | â | â |
| Sampedro et al. | 2017 | 260.204 | -36.103 | â | -1.1 | -0.1 | â |
| Joshi et al. | 2016 | 260.212 | -36.115 | â | â | â | â |
| Tadross | 2014 | 260.204 | -36.103 | â | â | â | â |
| Dias et al. | 2014 | 260.204 | -36.103 | â | -1.32 | -0.58 | -7.17 |
| Dias et al. | 2002 | 260.204 | -36.103 | â | -1.32 | -0.58 | -7.17 |
| Lynga | 1987 | 260.34 | -36.077 | â | â | â | 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 | 1.41 | 3.66 | 2.99 | 209 | 0.340 | 1546 | â | â |
| Hunt & Reffert | 2024 | 1.70 | 4.23 | 2.99 | 12 | â | 1546(1) | â | â |
| Cavallo et al. | 2024 | 1.69 | 3.91 | â | 12 | 0.340 | â | â | â |
| Hunt & Reffert | 2023 | 1.70 | 4.23 | 2.99 | 12 | â | â | â | â |
| Dib et al. | 2018 | 1.13 | â | â | 209 | â | â | â | â |
| Joshi et al. | 2016 | 1.13 | 3.25 | â | 209 | â | â | â | â |
| Tadross | 2014 | 1.02 | 3.34 | â | 500 | â | â | â | â |
| Dias et al. | 2002 | 1.02 | 3.34 | â | 501 | â | â | â | â |
| Lynga | 1987 | 2.30 | 3.66 | â | â | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Part of multiple system G17, along with HSC_2897, Bochum_13 and CWNU_1832.
Cavallo et al. (2024)
Bronze sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.04 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.04 (50th percentile).