NGC 6834

(MWSC 3197)

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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

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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

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

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 298.054 29.398 0.274 -2.494 -5.119 8.058
Almeida et al. 2025 298.053 29.4 – – – –
Hunt & Reffert 2024 298.054 29.395 0.271 -2.498 -5.112 10.512
Celli et al. 2024 298.052 29.399 – – – –
Cavallo et al. 2024 298.061 29.399 0.273 – – –
Hunt & Reffert 2023 298.054 29.395 0.271 -2.498 -5.112 10.512
Just et al. 2023 298.044 29.408 – – – –
Jaehnig et al. 2021 298.05 29.398 0.304 -2.484 -5.091 –
Rain et al. 2021 298.052 29.399 0.272 -2.487 -5.094 –
Dias et al. 2021 298.053 29.4 0.276 -2.49 -5.097 –
Cantat-Gaudin et al. 2020 298.052 29.399 0.272 -2.487 -5.094 –
Cantat-Gaudin & Anders 2020 298.052 29.399 0.272 -2.487 -5.094 –
Soubiran et al. 2018 298.052 29.399 – – – 11.09
Cantat-Gaudin et al. 2018 298.052 29.399 0.272 -2.487 -5.094 –
Loktin & Popova 2017 298.05 29.408 – -3.252 -3.894 -6.8
Kharchenko et al. 2016 298.044 29.408 – – – –
Dias et al. 2014 298.05 29.408 – -3.43 -3.16 –
Kharchenko et al. 2013 298.05 29.41 – -3.32 -4.31 -6.8
Gozha et al. 2012 298.05 29.408 – – – –
Kharchenko et al. 2007 298.05 29.41 – 0.04 – –
van den Bergh 2006 298.05 29.417 – – – –
Chen et al. 2003 298.04 29.416 – -0.12 -2.16 -6.8
Dias et al. 2002 298.05 29.408 – -3.43 -3.16 -6.8
Dambis 1999 298.05 29.408 – – – –

💡 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 – 14 – 1829 – –
Hunt & Reffert 2024 – – – – – 4556* – –
Celli et al. 2024 – – – 19 – 1733 – –
Cavallo et al. 2024 3.24 2.21 – 87 0.450 – – –
Hunt & Reffert 2023 3.20 2.38 2.17 22 – – – –
Just et al. 2023 – – – 95 – 118 – –
Jaehnig et al. 2021 3.30* – – – – – – –
Rain et al. 2021 3.33 2.17 – 76 – – – 0
Dias et al. 2021 2.96 2.23 – 14 0.024 – – –
Cantat-Gaudin et al. 2020 3.28 1.97 – 19 – – – –
Cantat-Gaudin & Anders 2020 3.33 – – – – – – –
Soubiran et al. 2018 3.33 – – – – – – –
Cantat-Gaudin et al. 2018 3.33 – – – – – – –
Loktin & Popova 2017 2.07 2.18 – 78 – – – –
Kharchenko et al. 2016 2.17 2.06 – 95 – – – –
Kharchenko et al. 2013 2.17 2.06 – 95 – – – –
Gozha et al. 2012 2.07 – – 76 – – – –
van den Bergh 2006 2.07 2.20 – 76 – – – –
Chen et al. 2003 2.07 – – 70 – – – –
Dias et al. 2002 2.07 2.19 – 76 – – – –
Dambis 1999 2.15 2.41 – 63 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0090 5.6 298.07 29.4 0.25 -2.48 -5.08 – 0.0

💡 Note: The % column shows the percentage of members that NGC 6834 shares with each listed object.

Visualization

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