NGC 146
(MWSC 59)
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
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
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 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 | β |
| Almeida et al. | 2025 | 8.259 | 63.33 | β | β | β | β |
| 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 | β | β | β |
| Hunt & Reffert | 2023 | 8.263 | 63.305 | 0.334 | -2.842 | -0.508 | -99.859 |
| Almeida et al. | 2023 | 8.251 | 63.325 | β | β | β | β |
| Just et al. | 2023 | 8.215 | 63.301 | β | β | β | β |
| Jaehnig et al. | 2021 | 8.207 | 63.318 | 0.352 | -2.825 | -0.434 | β |
| Rain et al. | 2021 | 8.262 | 63.316 | 0.307 | -2.864 | -0.451 | β |
| Dias et al. | 2021 | 8.259 | 63.33 | 0.311 | -2.873 | -0.458 | β |
| Cantat-Gaudin et al. | 2020 | 8.262 | 63.316 | 0.307 | -2.864 | -0.451 | β |
| SΓ‘nchez et al. | 2020 | 8.242 | 63.334 | β | -2.964 | -0.393 | β |
| Cantat-Gaudin & Anders | 2020 | 8.262 | 63.316 | 0.307 | -2.864 | -0.451 | β |
| Dias et al. | 2019 | 8.242 | 63.334 | 0.311 | -2.836 | -0.454 | 17.84 |
| Soubiran et al. | 2018 | 8.262 | 63.316 | β | β | β | 17.84 |
| Cantat-Gaudin et al. | 2018 | 8.262 | 63.316 | 0.307 | -2.864 | -0.451 | β |
| Loktin & Popova | 2017 | 8.235 | 63.334 | β | -2.754 | -1.393 | β |
| Kharchenko et al. | 2016 | 8.215 | 63.301 | β | β | β | β |
| Dias et al. | 2014 | 8.242 | 63.334 | β | -2.77 | 0.33 | β |
| Kharchenko et al. | 2013 | 8.226 | 63.305 | β | -4.17 | -2.23 | β |
| Kharchenko et al. | 2012 | 8.226 | 63.305 | β | -4.17 | -2.23 | β |
| Piskunov et al. | 2008 | 8.267 | 63.298 | β | β | β | β |
| van den Bergh | 2006 | 8.275 | 63.3 | β | β | β | β |
| Kharchenko et al. | 2005 | 8.26 | 63.3 | β | -2.41 | 0.89 | β |
| Kharchenko et al. | 2003 | 8.2 | 63.31 | β | -2.59 | 0.1 | β |
| Dias et al. | 2002 | 8.242 | 63.334 | β | -2.77 | 0.33 | β |
π‘ 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 | β | 48 | 0.056 | β | β | β |
| Almeida et al. | 2025 | 2.69 | 1.82 | β | 19 | β | 317 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 516* | β | β |
| Cavallo et al. | 2024 | 2.98 | 1.67 | β | 32 | 0.120 | β | β | β |
| Hunt & Reffert | 2023 | 2.77 | 1.61 | 0.49 | 17 | β | β | β | β |
| Almeida et al. | 2023 | 2.60 | 1.85 | β | 25 | -0.093 | 759* | 0.48 | β |
| Just et al. | 2023 | β | β | β | 50 | β | 481 | β | β |
| Jaehnig et al. | 2021 | 2.88* | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 2.97 | 1.71 | β | 13 | β | β | β | 0 |
| Dias et al. | 2021 | 2.69 | 1.82 | β | 19 | -0.051 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 3.15 | 1.60 | β | 35 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.97 | β | β | β | β | β | β | β |
| Dias et al. | 2019 | 2.73 | 1.33 | β | 32 | -1.112 | β | β | β |
| Soubiran et al. | 2018 | 2.97 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.97 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 3.05 | 1.46 | β | 68 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.80 | 1.86 | β | 50 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.80 | 1.86 | β | 50 | β | β | β | β |
| Kharchenko et al. | 2012 | 2.80 | 1.86 | β | 50 | β | β | β | β |
| Piskunov et al. | 2008 | 3.03 | 1.49 | β | 23 | β | β | β | β |
| van den Bergh | 2006 | 3.03 | 1.49 | β | 66 | β | β | β | β |
| Kharchenko et al. | 2005 | 3.03 | 1.49 | β | 23 | β | β | β | β |
| Kharchenko et al. | 2003 | 3.03 | 1.49 | β | β | β | β | β | β |
| Dias et al. | 2002 | 3.47 | 1.71 | β | 13 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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