NGC 559
(MWSC 122; FoF 551)
0.95
UTI
1.0
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
N50 (P>50% members)
1282
Stellar density (N50/rad)
60.3 [N/pc2]
- 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 metallicity and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 22.387 | 63.301 | 0.334 | -4.257 | 0.184 | -77.263 |
| Li et al. | 2025 | 22.387 | 63.301 | 0.325 | -4.258 | 0.254 | β |
| Carrasco-Varela et al. | 2025 | 22.717 | 63.365 | β | β | β | β |
| Almeida et al. | 2025 | 22.387 | 63.298 | β | β | β | β |
| 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 | β | β | β |
| Hunt & Reffert | 2023 | 22.389 | 63.304 | 0.334 | -4.276 | 0.191 | -77.171 |
| Almeida et al. | 2023 | 22.381 | 63.296 | β | β | β | β |
| Just et al. | 2023 | 22.368 | 63.299 | β | β | β | β |
| Jaehnig et al. | 2021 | 22.385 | 63.302 | 0.352 | -4.264 | 0.261 | β |
| Rain et al. | 2021 | 22.387 | 63.301 | 0.325 | -4.258 | 0.254 | β |
| 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 | β |
| SΓ‘nchez et al. | 2020 | 22.383 | 63.304 | β | -4.17 | 0.139 | β |
| Cantat-Gaudin & Anders | 2020 | 22.387 | 63.301 | 0.325 | -4.258 | 0.254 | β |
| Liu & Pang | 2019 | 22.382 | 63.295 | 0.326 | -4.239 | 0.25 | β |
| Soubiran et al. | 2018 | 22.387 | 63.301 | β | β | β | -77.25 |
| Cantat-Gaudin et al. | 2018 | 22.387 | 63.301 | 0.325 | -4.258 | 0.254 | β |
| Loktin & Popova | 2017 | 22.395 | 63.305 | β | -2.675 | -1.411 | -37.7 |
| Kharchenko et al. | 2016 | 22.368 | 63.299 | β | β | β | β |
| Dias et al. | 2014 | 22.396 | 63.304 | β | -4.58 | 1.41 | β |
| Kharchenko et al. | 2013 | 22.38 | 63.302 | β | -2.95 | -1.07 | -37.7 |
| Kharchenko et al. | 2012 | 22.38 | 63.302 | β | -3.19 | -1.28 | -37.7 |
| van den Bergh | 2006 | 22.34 | 63.28 | β | β | β | β |
| Dias et al. | 2002 | 22.383 | 63.304 | β | -4.58 | 1.41 | -58.4 |
| Dambis | 1999 | 22.325 | 63.283 | β | β | β | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 2.39 | 2.2 | 1.54 | 578 | -0.025 | 2621 | 0.71 | 0.01 |
| Li et al. | 2025 | 2.50 | 2.09 | β | 661 | 0.054 | β | β | β |
| Carrasco-Varela et al. | 2025 | 2.35 | 2.19 | β | 585 | -0.050 | β | β | 0.01(1) |
| Almeida et al. | 2025 | 2.35 | 2.19 | β | 585 | β | 3293 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 6156(1) | β | β |
| Cavallo et al. | 2024 | 2.78 | 2.41 | β | 339 | 0.230 | β | β | β |
| Hunt & Reffert | 2023 | 2.81 | 2.41 | 1.54 | 248 | β | β | β | β |
| Almeida et al. | 2023 | 2.35 | 2.21 | β | 571 | -0.095 | 1949(1) | 0.71 | β |
| Just et al. | 2023 | β | β | β | 631 | β | 1211 | β | β |
| Jaehnig et al. | 2021 | 2.87(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 2.83 | 2.54 | β | 224 | β | β | β | 1 |
| Dias et al. | 2021 | 2.35 | 2.19 | β | 585 | -0.025 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.88 | 2.19 | β | 257 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.83 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 1150 | 0.000 | β | β | β |
| Soubiran et al. | 2018 | 2.83 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.83 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.30 | 2.42 | β | 62 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.20 | 1.86 | β | 631 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.20 | 1.86 | β | 631 | β | β | β | β |
| Kharchenko et al. | 2012 | 2.20 | 1.86 | β | 631 | β | β | β | β |
| van den Bergh | 2006 | 1.26 | 2.45 | β | 56 | β | β | β | β |
| Dias et al. | 2002 | 2.43 | 2.54 | β | 224 | -0.250 | β | β | β |
| Dambis | 1999 | 1.99 | 2.30 | β | 45 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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