NGC 559

(MWSC 122; FoF 551)

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0.95 UTI
1.0
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members) 5.3 [arcmin]
  • CN 1.0 Very rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

NGC 559 is a very rich, very dense object of 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, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is very well-studied in the literature.
Relatively close Moderate extinction Massive Near-solar metallicity Intermediate age

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

Cavallo et al. (2024): Gold sample.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 22.387 63.301 0.334 -4.257 0.184 -77.263
Carrasco-Varela et al. 2025 22.717 63.365
Almeida et al. 2025 22.387 63.298
Hunt & Reffert 2024 22.389 63.304 0.334 -4.276 0.191 -77.171
Cavallo et al. 2024 22.396 63.297 0.333
Hunt & Reffert 2023 22.389 63.304 0.334 -4.276 0.191 -77.171
Just et al. 2023 22.368 63.299
Jaehnig et al. 2021 22.385 63.302 0.352 -4.264 0.261
Rain et al. 2021 22.387 63.301 0.325 -4.258 0.254
Dias et al. 2021 22.387 63.298 0.322 -4.253 0.245 -77.178
Cantat-Gaudin et al. 2020 22.387 63.301 0.325 -4.258 0.254
Liu & Pang 2019 22.382 63.295 0.326 -4.239 0.25
Soubiran et al. 2018 22.387 63.301 -77.25
Cantat-Gaudin et al. 2018 22.387 63.301 0.325 -4.258 0.254
Loktin & Popova 2017 22.395 63.305 -2.675 -1.411 -37.7
Kharchenko et al. 2016 22.368 63.299
Kharchenko et al. 2013 22.38 63.302 -2.95 -1.07 -37.7
Kharchenko et al. 2012 22.38 63.302 -3.19 -1.28 -37.7
Dias et al. 2002 22.383 63.304 -4.58 1.41 -58.4
Dambis 1999 22.325 63.283

💡 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
Carrasco-Varela et al. 2025 2.35 2.19 585 -0.050 0.01*
Almeida et al. 2025 2.35 2.19 585 3293
Hunt & Reffert 2024 6156*
Cavallo et al. 2024 2.78 2.41 339 0.230
Hunt & Reffert 2023 2.81 2.41 1.54 248
Just et al. 2023 631 1211
Jaehnig et al. 2021 2.87*
Rain et al. 2021 2.83 2.54 224 1
Dias et al. 2021 2.35 2.19 585 -0.025
Cantat-Gaudin et al. 2020 2.88 2.19 257
Liu & Pang 2019 1150 0.000
Soubiran et al. 2018 2.83
Cantat-Gaudin et al. 2018 2.83
Loktin & Popova 2017 1.30 2.42 62
Kharchenko et al. 2016 2.20 1.86 631
Kharchenko et al. 2013 2.20 1.86 631
Kharchenko et al. 2012 2.20 1.86 631
Dias et al. 2002 2.43 2.54 224 -0.250
Dambis 1999 1.99 2.30 45

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
(*): indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.