NGC 6846

(MWSC 3207)

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0.78 UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members) 0.9 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.7 Moderately studied
  • Cdup 1.0 Unique

Overview

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NGC 6846 is a rich, very dense object of high C3 quality. Its parallax locates it at a very large* distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, metal-poor, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~12.41 kpc) differs significantly from the median photometric distance (~5.32 kpc).

Very distant High extinction Massive Metal-poor Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 299.117 32.351 0.081 -2.884 -5.054 -43.175
Hunt & Reffert 2024 299.115 32.35 0.088 -2.873 -5.097 -42.508
Cavallo et al. 2024 299.101 32.337 0.09 – – –
Hunt & Reffert 2023 299.115 32.35 0.088 -2.873 -5.097 -42.508
Just et al. 2023 299.103 32.352 – – – –
Cantat-Gaudin et al. 2020 299.112 32.349 0.089 -2.971 -4.994 –
Cantat-Gaudin & Anders 2020 299.112 32.349 0.089 -2.971 -4.994 –
Soubiran et al. 2018 299.112 32.349 – – – -42.94
Cantat-Gaudin et al. 2018 299.112 32.349 0.089 -2.971 -4.994 –
Kharchenko et al. 2016 299.103 32.352 – – – –
Dias et al. 2014 299.117 32.348 – -0.05 -1.36 –
Kharchenko et al. 2013 299.109 32.355 – 0.12 -3.95 –
Dias et al. 2002 299.117 32.348 – 0.12 -3.95 –

💡 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
Hunt & Reffert 2024 – – – – – 2214* – –
Cavallo et al. 2024 4.51 3.92 – 178 -0.960 – – –
Hunt & Reffert 2023 9.14 4.18 2.39 44 – – – –
Just et al. 2023 – – – 1429 – 873 – –
Cantat-Gaudin et al. 2020 5.32 2.85 – 490 – – – –
Cantat-Gaudin & Anders 2020 8.50 – – – – – – –
Soubiran et al. 2018 8.50 – – – – – – –
Cantat-Gaudin et al. 2018 8.50 – – – – – – –
Kharchenko et al. 2016 4.45 3.25 – 1429 – – – –
Kharchenko et al. 2013 4.45 3.25 – 1429 – – – –
Dias et al. 2002 4.45 3.26 – 501 – – – –

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

Visualization

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