NGC 6823
(MWSC 3163)
0.96
UTI
0.8
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
3.7 [arcmin]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 6823 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is very well-studied in the literature.
Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate extinction
Massive
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 295.795 | 23.305 | 0.455 | -1.691 | -5.33 | 12.583 |
| Almeida et al. | 2025 | 295.796 | 23.331 | â | â | â | â |
| Hunt & Reffert | 2024 | 295.792 | 23.294 | 0.452 | -1.694 | -5.369 | 14.904 |
| Celli et al. | 2024 | 295.794 | 23.321 | â | â | â | â |
| Cavallo et al. | 2024 | 295.792 | 23.325 | 0.452 | â | â | â |
| Hunt & Reffert | 2023 | 295.792 | 23.294 | 0.452 | -1.694 | -5.369 | 14.904 |
| Just et al. | 2023 | 295.78 | 23.297 | â | â | â | â |
| Jaehnig et al. | 2021 | 295.788 | 23.32 | 0.477 | -1.718 | -5.317 | â |
| Rain et al. | 2021 | 295.794 | 23.321 | 0.446 | -1.697 | -5.304 | â |
| Dias et al. | 2021 | 295.796 | 23.331 | 0.445 | -1.69 | -5.299 | â |
| Cantat-Gaudin et al. | 2020 | 295.794 | 23.321 | 0.446 | -1.697 | -5.304 | â |
| Cantat-Gaudin & Anders | 2020 | 295.794 | 23.321 | 0.446 | -1.697 | -5.304 | â |
| Cantat-Gaudin et al. | 2018 | 295.794 | 23.321 | 0.446 | -1.697 | -5.304 | â |
| Loktin & Popova | 2017 | 295.8 | 23.3 | â | -2.688 | -2.861 | 10.5 |
| Kharchenko et al. | 2016 | 295.78 | 23.297 | â | â | â | â |
| Dias et al. | 2014 | 295.788 | 23.3 | â | -3.28 | -4.97 | â |
| Kharchenko et al. | 2013 | 295.785 | 23.3 | â | -3.0 | -4.0 | 10.5 |
| Gozha et al. | 2012 | 295.787 | 23.3 | â | â | â | â |
| Piskunov et al. | 2008 | 295.783 | 23.3 | â | â | â | â |
| Kharchenko et al. | 2007 | 295.78 | 23.3 | â | 0.27 | â | 17.0 |
| Piskunov et al. | 2007 | 295.783 | 23.3 | â | â | â | â |
| van den Bergh | 2006 | 295.792 | 23.298 | â | â | â | â |
| Kharchenko et al. | 2005 | 295.78 | 23.3 | â | -2.83 | -5.07 | 17.0 |
| Kharchenko et al. | 2003 | 295.78 | 23.28 | â | -2.35 | -5.78 | â |
| Chen et al. | 2003 | 295.745 | 23.32 | â | -1.41 | -3.04 | 11.0 |
| Dias et al. | 2002 | 295.788 | 23.3 | â | -1.41 | -3.04 | 13.59 |
| Dambis | 1999 | 295.787 | 23.3 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 2.08 | 2.52 | â | 7 | â | 1161 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1641* | â | â |
| Celli et al. | 2024 | â | â | â | 2 | â | 1370 | â | â |
| Cavallo et al. | 2024 | 1.80 | 2.38 | â | 8 | 0.020 | â | â | â |
| Hunt & Reffert | 2023 | 2.06 | 2.88 | 2.80 | 4 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 10 | â | 439 | â | â |
| Jaehnig et al. | 2021 | 2.10* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 2.10 | 2.63 | â | 3 | â | â | â | 0 |
| Dias et al. | 2021 | 2.08 | 2.52 | â | 7 | 0.127 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.33 | 2.22 | â | 2 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.10 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.10 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.89 | 2.61 | â | 7 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.76 | 2.58 | â | 10 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.76 | 2.58 | â | 10 | â | â | â | â |
| Gozha et al. | 2012 | 3.18 | â | â | 3 | 0.080 | 10000 | â | â |
| Piskunov et al. | 2008 | 1.89 | 2.60 | â | 10 | â | 2838* | â | â |
| Piskunov et al. | 2007 | 1.89 | 2.60 | â | 10 | â | 409 | â | â |
| van den Bergh | 2006 | 1.89 | 2.60 | â | 7 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.89 | 2.60 | â | 10 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.89 | 2.02 | â | â | â | â | â | â |
| Chen et al. | 2003 | 1.89 | â | â | 0 | â | â | â | â |
| Dias et al. | 2002 | 3.18 | 2.65 | â | 3 | â | â | â | â |
| Dambis | 1999 | 1.91 | 2.64 | â | 3 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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