NGC 146

(MWSC 59)

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0.94 UTI
0.7
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members) 3.6 [arcmin]
  • CN 0.7 Moderately populated
  • 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 146 is a moderately populated, 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 near-solar metallicity, young cluster (see Parameters). It is very well-studied in the literature.

Note: This object shares a small percentage of members with 2 later reported entries. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good 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 – 8.24 63.314 0.331 -2.847 -0.491 -99.852
Li et al. 2025 8.262 63.316 0.307 -2.864 -0.451 –
Almeida et al. 2025 8.259 63.33 – – – –
Hunt & Reffert 2024 8.263 63.305 0.334 -2.842 -0.508 -99.859
Cavallo et al. 2024 8.254 63.326 0.334 – – –
Hunt & Reffert 2023 8.263 63.305 0.334 -2.842 -0.508 -99.859
Almeida et al. 2023 8.251 63.325 – – – –
Just et al. 2023 8.215 63.301 – – – –
Jaehnig et al. 2021 8.207 63.318 0.352 -2.825 -0.434 –
Rain et al. 2021 8.262 63.316 0.307 -2.864 -0.451 –
Dias et al. 2021 8.259 63.33 0.311 -2.873 -0.458 –
Cantat-Gaudin et al. 2020 8.262 63.316 0.307 -2.864 -0.451 –
SΓ‘nchez et al. 2020 8.242 63.334 – -2.964 -0.393 –
Cantat-Gaudin & Anders 2020 8.262 63.316 0.307 -2.864 -0.451 –
Dias et al. 2019 8.242 63.334 0.311 -2.836 -0.454 17.84
Soubiran et al. 2018 8.262 63.316 – – – 17.84
Cantat-Gaudin et al. 2018 8.262 63.316 0.307 -2.864 -0.451 –
Loktin & Popova 2017 8.235 63.334 – -2.754 -1.393 –
Kharchenko et al. 2016 8.215 63.301 – – – –
Dias et al. 2014 8.242 63.334 – -2.77 0.33 –
Kharchenko et al. 2013 8.226 63.305 – -4.17 -2.23 –
Kharchenko et al. 2012 8.226 63.305 – -4.17 -2.23 –
Piskunov et al. 2008 8.267 63.298 – – – –
van den Bergh 2006 8.275 63.3 – – – –
Kharchenko et al. 2005 8.26 63.3 – -2.41 0.89 –
Kharchenko et al. 2003 8.2 63.31 – -2.59 0.1 –
Dias et al. 2002 8.242 63.334 – -2.77 0.33 –

πŸ’‘ 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 2.79 1.71 – 48 0.056 – – –
Almeida et al. 2025 2.69 1.82 – 19 – 317 – –
Hunt & Reffert 2024 – – – – – 516* – –
Cavallo et al. 2024 2.98 1.67 – 32 0.120 – – –
Hunt & Reffert 2023 2.77 1.61 0.49 17 – – – –
Almeida et al. 2023 2.60 1.85 – 25 -0.093 759* 0.48 –
Just et al. 2023 – – – 50 – 481 – –
Jaehnig et al. 2021 2.88* – – – – – – –
Rain et al. 2021 2.97 1.71 – 13 – – – 0
Dias et al. 2021 2.69 1.82 – 19 -0.051 – – –
Cantat-Gaudin et al. 2020 3.15 1.60 – 35 – – – –
Cantat-Gaudin & Anders 2020 2.97 – – – – – – –
Dias et al. 2019 2.73 1.33 – 32 -1.112 – – –
Soubiran et al. 2018 2.97 – – – – – – –
Cantat-Gaudin et al. 2018 2.97 – – – – – – –
Loktin & Popova 2017 3.05 1.46 – 68 – – – –
Kharchenko et al. 2016 2.80 1.86 – 50 – – – –
Kharchenko et al. 2013 2.80 1.86 – 50 – – – –
Kharchenko et al. 2012 2.80 1.86 – 50 – – – –
Piskunov et al. 2008 3.03 1.49 – 23 – – – –
van den Bergh 2006 3.03 1.49 – 66 – – – –
Kharchenko et al. 2005 3.03 1.49 – 23 – – – –
Kharchenko et al. 2003 3.03 1.49 – – – – – –
Dias et al. 2002 3.47 1.71 – 13 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 10480 18.0 8.34 63.32 0.33 -2.82 -0.55 – 0.13
FoF 1864 2.2 8.7 63.04 0.35 -2.91 -0.56 – 0.08

πŸ’‘ Note: The % column shows the percentage of members that NGC 146 shares with each listed object.

Visualization

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