NGC 6793
(MWSC 3098; OCL 115; FoF 2338)
0.98
UTI
0.88
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
16.0 [arcmin]
- CN 0.88 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 6793 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.
Close
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 290.807 | 22.152 | 1.668 | 3.797 | 3.538 | -19.658 |
| Li et al. | 2025 | 290.817 | 22.159 | 1.669 | 3.795 | 3.544 | â |
| Wei et al. | 2025 | 290.818 | 22.152 | 1.675 | 3.796 | 3.548 | â |
| Almeida et al. | 2025 | 290.801 | 22.173 | â | â | â | â |
| Alfonso et al. | 2024 | 290.808 | 22.141 | 1.647 | 3.788 | 3.529 | â |
| Hunt & Reffert | 2024 | 290.818 | 22.164 | 1.671 | 3.8 | 3.536 | -20.021 |
| Cavallo et al. | 2024 | 290.81 | 22.137 | 1.674 | â | â | â |
| Hunt & Reffert | 2023 | 290.818 | 22.164 | 1.671 | 3.8 | 3.536 | -20.021 |
| Almeida et al. | 2023 | 290.803 | 22.172 | â | â | â | â |
| Just et al. | 2023 | 290.818 | 22.138 | â | â | â | â |
| He et al. | 2022 | 290.808 | 22.148 | 1.678 | 3.795 | 3.552 | â |
| Tarricq et al. | 2022 | 290.833 | 22.145 | 1.679 | 3.789 | 3.544 | â |
| Dias et al. | 2021 | 290.801 | 22.173 | 1.667 | 3.778 | 3.569 | -25.681 |
| Cantat-Gaudin et al. | 2020 | 290.817 | 22.159 | 1.669 | 3.795 | 3.544 | â |
| Cantat-Gaudin & Anders | 2020 | 290.817 | 22.159 | 1.669 | 3.795 | 3.544 | â |
| Liu & Pang | 2019 | 290.816 | 22.13 | 1.67 | 3.774 | 3.577 | â |
| Bossini et al. | 2019 | 290.817 | 22.159 | â | â | â | â |
| Soubiran et al. | 2018 | 290.817 | 22.159 | â | â | â | -16.59 |
| Bica et al. | 2019 | 290.836 | 22.154 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 290.817 | 22.159 | 1.669 | 3.795 | 3.544 | â |
| Loktin & Popova | 2017 | 290.79 | 22.155 | â | 0.639 | -6.083 | â |
| Kharchenko et al. | 2016 | 290.818 | 22.138 | â | â | â | â |
| Dias et al. | 2014 | 290.808 | 22.142 | â | 2.9 | 1.41 | â |
| Kharchenko et al. | 2013 | 290.824 | 22.14 | â | 4.8 | 1.69 | â |
| Piskunov et al. | 2008 | 290.802 | 22.137 | â | â | â | â |
| Kharchenko et al. | 2005 | 290.8 | 22.14 | â | 3.9 | 1.09 | â |
| Kharchenko et al. | 2003 | 290.8 | 22.16 | â | 4.87 | 1.37 | â |
| Dias et al. | 2002 | 290.808 | 22.142 | â | 2.9 | 1.41 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 0.55 | 0.89 | â | 377 | 0.150 | â | â | â |
| Wei et al. | 2025 | 0.61 | 0.61 | â | 251 | 0.500 | 504 | 0.22 | â |
| Almeida et al. | 2025 | 0.59 | 1.01 | â | 458 | â | 408 | â | â |
| Alfonso et al. | 2024 | 0.63 | 0.74 | â | 417 | 0.234 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 625* | â | â |
| Cavallo et al. | 2024 | 0.59 | 1.09 | â | 240 | 0.390 | â | â | â |
| Hunt & Reffert | 2023 | 0.57 | 1.03 | 1.23 | 136 | â | â | â | â |
| Almeida et al. | 2023 | 0.58 | 1.17 | â | 329 | 0.126 | 409* | 0.48 | â |
| Just et al. | 2023 | â | â | â | 495 | â | 32 | â | â |
| He et al. | 2022 | â | 1.40 | â | 71 | â | â | â | â |
| Tarricq et al. | 2022 | 0.62 | â | â | 309 | â | â | â | â |
| Dias et al. | 2021 | 0.59 | 1.01 | â | 458 | 0.234 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.63 | 0.74 | â | 309 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.59 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 66 | 0.250 | â | â | â |
| Bossini et al. | 2019 | 0.54 | 0.68 | â | 573 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.59 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.59 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.68 | 1.50 | â | 851 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.72 | 0.97 | â | 495 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.72 | 0.97 | â | 495 | â | â | â | â |
| Piskunov et al. | 2008 | 1.10 | 0.53 | â | 437 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.10 | 0.53 | â | 437 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.91 | 0.62 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.10 | 0.53 | â | 437 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.