NGC 2335
(MWSC 1100; FoF 2080; CMa19)
0.91
UTI
0.81
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
6.8 [arcmin]
- CN 0.81 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 2335 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 moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (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 | 106.688 | -10.03 | 0.579 | -0.798 | -0.634 | 23.85 |
| Li et al. | 2025 | 106.69 | -10.023 | 0.585 | -0.784 | -0.642 | β |
| Almeida et al. | 2025 | 106.679 | -10.015 | β | β | β | β |
| Hunt & Reffert | 2024 | 106.723 | -10.041 | 0.574 | -0.789 | -0.628 | 24.277 |
| Cavallo et al. | 2024 | 106.675 | -10.017 | 0.582 | β | β | β |
| Hunt & Reffert | 2023 | 106.723 | -10.041 | 0.574 | -0.789 | -0.628 | 24.277 |
| Just et al. | 2023 | 106.704 | -10.028 | β | β | β | β |
| Jaehnig et al. | 2021 | 106.694 | -10.029 | 0.618 | -0.779 | -0.662 | β |
| Santos-Silva et al. | 2021 | 106.67 | -10.03 | 0.58 | -0.77 | -0.66 | β |
| Rain et al. | 2021 | 106.69 | -10.023 | 0.585 | -0.784 | -0.642 | β |
| Dias et al. | 2021 | 106.679 | -10.015 | 0.581 | -0.793 | -0.658 | β |
| Cantat-Gaudin et al. | 2020 | 106.69 | -10.023 | 0.585 | -0.784 | -0.642 | β |
| SΓ‘nchez et al. | 2020 | 106.704 | -10.028 | β | -0.798 | -0.586 | β |
| Cantat-Gaudin & Anders | 2020 | 106.69 | -10.023 | 0.585 | -0.784 | -0.642 | β |
| Liu & Pang | 2019 | 106.7 | -10.014 | 0.571 | -0.791 | -0.654 | β |
| Cantat-Gaudin et al. | 2018 | 106.69 | -10.023 | 0.585 | -0.784 | -0.642 | β |
| Loktin & Popova | 2017 | 106.71 | -10.027 | β | -1.9 | -2.647 | 8.7 |
| Kharchenko et al. | 2016 | 106.704 | -10.028 | β | β | β | β |
| Dias et al. | 2014 | 106.704 | -10.028 | β | 0.37 | -2.34 | β |
| Kharchenko et al. | 2013 | 106.71 | -10.03 | β | 0.2 | -2.99 | 8.7 |
| Gozha et al. | 2012 | 106.704 | -10.028 | β | β | β | β |
| Piskunov et al. | 2008 | 106.706 | -10.027 | β | β | β | β |
| Kharchenko et al. | 2007 | 106.71 | -10.03 | β | 0.25 | β | 8.7 |
| Piskunov et al. | 2007 | 106.706 | -10.027 | β | β | β | β |
| van den Bergh | 2006 | 106.704 | -10.028 | β | β | β | β |
| Kharchenko et al. | 2005 | 106.71 | -10.03 | β | 1.45 | -3.31 | β |
| Kharchenko et al. | 2003 | 106.71 | -10.05 | β | 0.98 | -2.38 | β |
| Chen et al. | 2003 | 106.716 | -10.045 | β | β | β | β |
| Dias et al. | 2002 | 106.704 | -10.028 | β | -0.91 | -3.18 | -3.59 |
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 | 1.455 | 1.22 | 2.41 | 158 | -0.030 | 700 | β | 0.0 |
| Li et al. | 2025 | 1.54 | 1.39 | β | 107 | -0.142 | β | β | β |
| Almeida et al. | 2025 | 1.46 | 1.48 | β | 65 | β | 693 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 985(1) | β | β |
| Cavallo et al. | 2024 | 1.73 | 1.26 | β | 219 | 0.560 | β | β | β |
| Hunt & Reffert | 2023 | 1.59 | 1.36 | 2.41 | 148 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 158 | β | 468 | β | β |
| Jaehnig et al. | 2021 | 1.60(1) | β | β | β | β | β | β | β |
| Santos-Silva et al. | 2021 | 1.45(1) | 1.54(1) | β | 42(1) | -0.090(1) | β | β | β |
| Rain et al. | 2021 | 1.63 | 1.21 | β | 162 | β | β | β | 0 |
| Dias et al. | 2021 | 1.46 | 1.48 | β | 65 | -0.071 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.66 | 0.83 | β | 324 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.63 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 355 | 0.250 | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.63 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.47 | 1.22 | β | 171 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.41 | 1.29 | β | 158 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.41 | 1.29 | β | 158 | -0.030 | β | β | β |
| Gozha et al. | 2012 | 1.42 | β | β | 162 | 0.080 | 776 | β | β |
| Piskunov et al. | 2008 | 1.42 | 1.21 | β | 120 | β | 708(1) | β | β |
| Piskunov et al. | 2007 | 1.42 | 1.21 | β | 120 | β | 136 | β | β |
| van den Bergh | 2006 | 1.42 | 1.21 | β | 162 | β | β | β | β |
| Kharchenko et al. | 2005 | 1.42 | 1.21 | β | 120 | β | β | β | β |
| Kharchenko et al. | 2003 | 1.41 | 1.21 | β | β | β | β | β | β |
| Chen et al. | 2003 | 1.42 | 1.22 | β | 160 | -0.030(1) | β | β | β |
| Dias et al. | 2002 | 1.42 | 1.22 | β | 162 | -0.180 | β | β | β |
(N): Indicates that are N extra values assigned to this parameter in the corresponding reference.


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