NGC 1960
(MWSC 594)
0.92
UTI
0.87
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
134.8 [N/pc2]
- CN 0.87 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 1960 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is very well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 84.086 | 34.137 | 0.842 | -0.221 | -3.401 | -3.23 |
| Li et al. | 2025 | 84.084 | 34.135 | 0.835 | -0.155 | -3.388 | β |
| Almeida et al. | 2025 | 84.079 | 34.134 | β | β | β | β |
| Zhang et al. | 2024 | 84.085 | 34.134 | β | β | β | β |
| Hunt & Reffert | 2024 | 84.085 | 34.134 | 0.843 | -0.218 | -3.414 | -5.135 |
| Celli et al. | 2024 | 84.084 | 34.135 | β | β | β | β |
| Cavallo et al. | 2024 | 84.086 | 34.134 | 0.844 | β | β | β |
| Hunt & Reffert | 2023 | 84.085 | 34.134 | 0.843 | -0.218 | -3.414 | -5.135 |
| Almeida et al. | 2023 | 84.084 | 34.131 | β | β | β | β |
| Just et al. | 2023 | 84.073 | 34.159 | β | β | β | β |
| He et al. | 2022 | 84.085 | 34.134 | 0.845 | -0.219 | -3.406 | β |
| Jaehnig et al. | 2021 | 84.089 | 34.137 | 0.868 | -0.162 | -3.372 | β |
| Rain et al. | 2021 | 84.084 | 34.135 | 0.835 | -0.155 | -3.388 | β |
| Dias et al. | 2021 | 84.079 | 34.134 | 0.832 | -0.146 | -3.395 | β |
| Cantat-Gaudin et al. | 2020 | 84.084 | 34.135 | 0.835 | -0.155 | -3.388 | β |
| SΓ‘nchez et al. | 2020 | 84.075 | 34.14 | β | -0.02 | -3.339 | β |
| Cantat-Gaudin & Anders | 2020 | 84.084 | 34.135 | 0.835 | -0.155 | -3.388 | β |
| Bossini et al. | 2019 | 84.084 | 34.135 | β | β | β | β |
| Soubiran et al. | 2018 | 84.084 | 34.135 | β | β | β | 7.03 |
| Cantat-Gaudin et al. | 2018 | 84.084 | 34.135 | 0.835 | -0.155 | -3.388 | β |
| Loktin & Popova | 2017 | 84.075 | 34.14 | β | 0.364 | -1.456 | -1.2 |
| Kharchenko et al. | 2016 | 84.073 | 34.159 | β | β | β | β |
| Dias et al. | 2014 | 84.075 | 34.14 | β | -0.22 | -5.66 | β |
| Kharchenko et al. | 2013 | 84.082 | 34.158 | β | 0.91 | -4.35 | -1.2 |
| Gozha et al. | 2012 | 84.075 | 34.14 | β | β | β | β |
| Kharchenko et al. | 2012 | 84.082 | 34.158 | β | 0.91 | -4.35 | -1.18 |
| Piskunov et al. | 2008 | 84.07 | 34.143 | β | β | β | β |
| Kharchenko et al. | 2007 | 84.07 | 34.14 | β | 0.27 | β | -1.18 |
| Piskunov et al. | 2007 | 84.07 | 34.143 | β | β | β | β |
| van den Bergh | 2006 | 84.05 | 34.14 | β | β | β | β |
| Kharchenko et al. | 2005 | 84.07 | 34.14 | β | 0.5 | -4.94 | -1.18 |
| Kharchenko et al. | 2003 | 84.06 | 34.15 | β | 0.02 | -5.14 | β |
| Chen et al. | 2003 | 83.979 | 34.13 | β | 1.1 | -4.08 | -4.0 |
| Dias et al. | 2002 | 84.075 | 34.14 | β | -0.22 | -5.66 | -17.83 |
| Dambis | 1999 | 84.075 | 34.14 | 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 | 1.16 | 0.71 | 0.93 | 28 | -0.028 | 688 | 0.53 | 0.0 |
| Li et al. | 2025 | 1.06 | 0.80 | β | 23 | -0.145 | β | β | β |
| Almeida et al. | 2025 | 1.09 | 0.93 | β | 30 | β | 759 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.191(1) | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1316(1) | β | β |
| Celli et al. | 2024 | β | β | β | 28 | β | 886 | β | β |
| Cavallo et al. | 2024 | 1.18 | 0.77 | β | 25 | 0.030 | β | β | β |
| Hunt & Reffert | 2023 | 1.12 | 0.79 | 0.93 | 27 | β | β | β | β |
| Almeida et al. | 2023 | 1.12 | 0.90 | β | 28 | -0.026 | 629(1) | 0.53 | β |
| Just et al. | 2023 | β | β | β | 37 | β | 163 | β | β |
| He et al. | 2022 | β | 1.00 | β | 20 | β | β | β | β |
| Jaehnig et al. | 2021 | 1.15(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 1.16 | 0.65 | β | 25 | β | β | β | 0 |
| Dias et al. | 2021 | 1.09 | 0.93 | β | 30 | -0.030 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.16 | 0.63 | β | 28 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.16 | β | β | β | β | β | β | β |
| Bossini et al. | 2019 | 1.13 | 0.66 | β | 26 | 0.000 | β | β | β |
| Soubiran et al. | 2018 | 1.16 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.16 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.33 | 0.70 | β | 28 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.20 | 0.78 | β | 37 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.20 | 0.78 | β | 37 | β | β | β | β |
| Gozha et al. | 2012 | 1.33 | β | β | 25 | β | 309 | β | β |
| Kharchenko et al. | 2012 | 1.20 | 0.78 | β | 37 | β | β | β | β |
| Piskunov et al. | 2008 | 1.32 | 0.68 | β | 42 | β | 746(1) | β | β |
| Piskunov et al. | 2007 | 1.32 | 0.68 | β | 42 | β | 191 | β | β |
| van den Bergh | 2006 | 1.32 | 0.68 | β | 30 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.32 | 0.68 | β | 42 | β | β | β | β |
| Kharchenko et al. | 2003 | 0.72 | 0.68 | β | β | β | β | β | β |
| Chen et al. | 2003 | 1.32 | β | β | 20 | β | β | β | β |
| Dias et al. | 2002 | 1.33 | 0.68 | β | 25 | β | β | β | β |
| Dambis | 1999 | 1.10 | 0.71 | β | 16 | 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: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.