NGC 6834
(MWSC 3197)
0.98
UTI
0.88
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
3.4 [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 6834 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, young cluster, but with a large variance across recent sources for the age 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.
Relatively close
Moderate extinction
Massive
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 298.054 | 29.398 | 0.274 | -2.494 | -5.119 | 8.058 |
| Almeida et al. | 2025 | 298.053 | 29.4 | â | â | â | â |
| Hunt & Reffert | 2024 | 298.054 | 29.395 | 0.271 | -2.498 | -5.112 | 10.512 |
| Celli et al. | 2024 | 298.052 | 29.399 | â | â | â | â |
| Cavallo et al. | 2024 | 298.061 | 29.399 | 0.273 | â | â | â |
| Hunt & Reffert | 2023 | 298.054 | 29.395 | 0.271 | -2.498 | -5.112 | 10.512 |
| Just et al. | 2023 | 298.044 | 29.408 | â | â | â | â |
| Jaehnig et al. | 2021 | 298.05 | 29.398 | 0.304 | -2.484 | -5.091 | â |
| Rain et al. | 2021 | 298.052 | 29.399 | 0.272 | -2.487 | -5.094 | â |
| Dias et al. | 2021 | 298.053 | 29.4 | 0.276 | -2.49 | -5.097 | â |
| Cantat-Gaudin et al. | 2020 | 298.052 | 29.399 | 0.272 | -2.487 | -5.094 | â |
| Cantat-Gaudin & Anders | 2020 | 298.052 | 29.399 | 0.272 | -2.487 | -5.094 | â |
| Soubiran et al. | 2018 | 298.052 | 29.399 | â | â | â | 11.09 |
| Cantat-Gaudin et al. | 2018 | 298.052 | 29.399 | 0.272 | -2.487 | -5.094 | â |
| Loktin & Popova | 2017 | 298.05 | 29.408 | â | -3.252 | -3.894 | -6.8 |
| Kharchenko et al. | 2016 | 298.044 | 29.408 | â | â | â | â |
| Dias et al. | 2014 | 298.05 | 29.408 | â | -3.43 | -3.16 | â |
| Kharchenko et al. | 2013 | 298.05 | 29.41 | â | -3.32 | -4.31 | -6.8 |
| Gozha et al. | 2012 | 298.05 | 29.408 | â | â | â | â |
| Kharchenko et al. | 2007 | 298.05 | 29.41 | â | 0.04 | â | â |
| van den Bergh | 2006 | 298.05 | 29.417 | â | â | â | â |
| Chen et al. | 2003 | 298.04 | 29.416 | â | -0.12 | -2.16 | -6.8 |
| Dias et al. | 2002 | 298.05 | 29.408 | â | -3.43 | -3.16 | -6.8 |
| Dambis | 1999 | 298.05 | 29.408 | 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 | 2.96 | 2.23 | â | 14 | â | 1829 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 4556* | â | â |
| Celli et al. | 2024 | â | â | â | 19 | â | 1733 | â | â |
| Cavallo et al. | 2024 | 3.24 | 2.21 | â | 87 | 0.450 | â | â | â |
| Hunt & Reffert | 2023 | 3.20 | 2.38 | 2.17 | 22 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 95 | â | 118 | â | â |
| Jaehnig et al. | 2021 | 3.30* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 3.33 | 2.17 | â | 76 | â | â | â | 0 |
| Dias et al. | 2021 | 2.96 | 2.23 | â | 14 | 0.024 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.28 | 1.97 | â | 19 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.33 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 3.33 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.33 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.07 | 2.18 | â | 78 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.17 | 2.06 | â | 95 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.17 | 2.06 | â | 95 | â | â | â | â |
| Gozha et al. | 2012 | 2.07 | â | â | 76 | â | â | â | â |
| van den Bergh | 2006 | 2.07 | 2.20 | â | 76 | â | â | â | â |
| Chen et al. | 2003 | 2.07 | â | â | 70 | â | â | â | â |
| Dias et al. | 2002 | 2.07 | 2.19 | â | 76 | â | â | â | â |
| Dambis | 1999 | 2.15 | 2.41 | â | 63 | 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)
Gold sample.