NGC 581
(MWSC 124; FoF 2131)
0.96
UTI
0.79
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
29.5 [N/pc2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 581 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below 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 5 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 23.341 | 60.661 | 0.362 | -1.397 | -0.581 | -38.143 |
| Li et al. | 2025 | 23.339 | 60.659 | 0.373 | -1.384 | -0.497 | â |
| Almeida et al. | 2025 | 23.331 | 60.66 | â | â | â | â |
| Hunt & Reffert | 2024 | 23.36 | 60.656 | 0.366 | -1.394 | -0.598 | -38.142 |
| Celli et al. | 2024 | 23.339 | 60.659 | â | â | â | â |
| Cavallo et al. | 2024 | 23.327 | 60.66 | 0.366 | â | â | â |
| Hunt & Reffert | 2023 | 23.36 | 60.656 | 0.366 | -1.394 | -0.598 | -38.142 |
| Almeida et al. | 2023 | 23.342 | 60.661 | â | â | â | â |
| Just et al. | 2023 | 23.305 | 60.649 | â | â | â | â |
| Jaehnig et al. | 2021 | 23.331 | 60.658 | 0.4 | -1.389 | -0.504 | â |
| Rain et al. | 2021 | 23.339 | 60.659 | 0.373 | -1.384 | -0.497 | â |
| Dias et al. | 2021 | 23.331 | 60.66 | 0.374 | -1.383 | -0.493 | â |
| Cantat-Gaudin et al. | 2020 | 23.339 | 60.659 | 0.373 | -1.384 | -0.497 | â |
| Cantat-Gaudin & Anders | 2020 | 23.339 | 60.659 | 0.373 | -1.384 | -0.497 | â |
| Liu & Pang | 2019 | 23.293 | 60.638 | 0.455 | -1.367 | -0.544 | â |
| Dias et al. | 2019 | 23.346 | 60.65 | 0.37 | -1.382 | -0.504 | -45.33 |
| Bossini et al. | 2019 | 23.339 | 60.659 | â | â | â | â |
| Soubiran et al. | 2018 | 23.339 | 60.659 | â | â | â | -45.33 |
| Cantat-Gaudin et al. | 2018 | 23.339 | 60.659 | 0.373 | -1.384 | -0.497 | â |
| Loktin & Popova | 2017 | 23.34 | 60.65 | â | -0.263 | -0.467 | -41.4 |
| Kharchenko et al. | 2016 | 23.305 | 60.649 | â | â | â | â |
| Dias et al. | 2014 | 23.346 | 60.65 | â | -1.86 | -0.46 | â |
| Kharchenko et al. | 2013 | 23.316 | 60.652 | â | -1.14 | 0.37 | -41.4 |
| Gozha et al. | 2012 | 23.346 | 60.65 | â | â | â | â |
| Kharchenko et al. | 2012 | 23.316 | 60.652 | â | -1.14 | 0.37 | -41.43 |
| Piskunov et al. | 2008 | 23.339 | 60.645 | â | â | â | â |
| Kharchenko et al. | 2007 | 23.34 | 60.65 | â | 0.12 | â | -41.43 |
| van den Bergh | 2006 | 23.35 | 60.65 | â | â | â | â |
| Kharchenko et al. | 2005 | 23.34 | 60.65 | â | -0.69 | 0.2 | -40.42 |
| Kharchenko et al. | 2003 | 23.34 | 60.67 | â | -0.02 | 0.03 | â |
| Chen et al. | 2003 | 23.242 | 60.662 | â | -1.6 | 0.66 | -37.0 |
| Dias et al. | 2002 | 23.346 | 60.65 | â | -1.6 | 0.66 | -44.2 |
| Dambis | 1999 | 23.346 | 60.65 | â | â | â | â |
đĄ 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 | 99999â | 2.29 | 1.195 | 0.93 | 28 | -0.049 | 720 | 0.7 | 0.0 |
| Li et al. | 2025 | 2.42 | 1.35 | â | 24 | 0.046 | â | â | â |
| Almeida et al. | 2025 | 2.29 | 1.45 | â | 29 | â | 831 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1262(1) | â | â |
| Celli et al. | 2024 | â | â | â | 28 | â | 725 | â | â |
| Cavallo et al. | 2024 | 2.74 | 1.58 | â | 22 | -0.100 | â | â | â |
| Hunt & Reffert | 2023 | 2.50 | 1.29 | 0.93 | 47 | â | â | â | â |
| Almeida et al. | 2023 | 2.33 | 1.41 | â | 66 | -0.078 | 715(1) | 0.70 | â |
| Just et al. | 2023 | â | â | â | 28 | â | 404 | â | â |
| Jaehnig et al. | 2021 | 2.48(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 2.49 | 1.18 | â | 21 | â | â | â | 0 |
| Dias et al. | 2021 | 2.29 | 1.45 | â | 29 | -0.020 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.50 | 1.09 | â | 28 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.49 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 60 | 0.500 | â | â | â |
| Dias et al. | 2019 | 2.06 | 1.05 | â | 22 | -1.623 | â | â | â |
| Bossini et al. | 2019 | 2.65 | 1.21 | â | 26 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 2.49 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.49 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.20 | 1.17 | â | 22 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.20 | 1.03 | â | 28 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.20 | 1.03 | â | 28 | â | â | â | â |
| Gozha et al. | 2012 | 2.19 | â | â | 22 | -0.850 | 178 | â | â |
| Kharchenko et al. | 2012 | 2.20 | 1.03 | â | 28 | â | â | â | â |
| Piskunov et al. | 2008 | 2.19 | 1.21 | â | 28 | â | â | â | â |
| van den Bergh | 2006 | 2.19 | 1.18 | â | 22 | â | â | â | â |
| Kharchenko et al. | 2005 | 2.19 | 1.21 | â | 28 | â | â | â | â |
| Kharchenko et al. | 2003 | 2.17 | 1.18 | â | â | â | â | â | â |
| Chen et al. | 2003 | 2.19 | â | â | 20 | â | â | â | â |
| Dias et al. | 2002 | 2.19 | 1.18 | â | 22 | â | â | â | â |
| Dambis | 1999 | 2.61 | 1.28 | â | 16 | â | â | â | â |
(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. Silver sample.
Cavallo et al. (2024)
Gold sample.