NGC 6405
(MWSC 2661; FoF 2415; OCSN 239)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
202.6 [N/pc2]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
NGC 6405 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a very 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 absorption, metallicity, and mass 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 | 99999â | 265.091 | -32.234 | 2.176 | -1.355 | -5.862 | -10.491 |
| Li et al. | 2025 | 265.069 | -32.242 | 2.172 | -1.306 | -5.847 | â |
| Wei et al. | 2025 | 265.083 | -32.245 | 2.183 | -1.381 | -5.875 | â |
| Almeida et al. | 2025 | 265.104 | -32.24 | â | â | â | â |
| Alfonso et al. | 2024 | 265.095 | -32.23 | 2.14 | -1.362 | -5.866 | â |
| Hunt & Reffert | 2024 | 265.067 | -32.228 | 2.177 | -1.368 | -5.847 | -10.527 |
| Cavallo et al. | 2024 | 265.075 | -32.224 | 2.174 | â | â | â |
| Hunt & Reffert | 2023 | 265.067 | -32.228 | 2.177 | -1.368 | -5.847 | -10.527 |
| Qin et al. | 2023 | 265.04 | -32.23 | 2.17 | -1.37 | -5.87 | -10.51 |
| Just et al. | 2023 | 265.071 | -32.215 | â | â | â | â |
| He et al. | 2022 | 265.069 | -32.249 | 2.177 | -1.354 | -5.858 | â |
| Jaehnig et al. | 2021 | 265.12 | -32.238 | 2.196 | -1.328 | -5.815 | â |
| Rain et al. | 2021 | 265.069 | -32.242 | 2.172 | -1.306 | -5.847 | â |
| Dias et al. | 2021 | 265.104 | -32.24 | 2.167 | -1.312 | -5.839 | -8.71 |
| Cantat-Gaudin et al. | 2020 | 265.069 | -32.242 | 2.172 | -1.306 | -5.847 | â |
| Cantat-Gaudin & Anders | 2020 | 265.069 | -32.242 | 2.172 | -1.306 | -5.847 | â |
| Liu & Pang | 2019 | 265.089 | -32.257 | 2.16 | -1.339 | -5.846 | â |
| Soubiran et al. | 2018 | 265.069 | -32.242 | â | â | â | -9.47 |
| Cantat-Gaudin et al. | 2018 | 265.069 | -32.242 | 2.172 | -1.306 | -5.847 | â |
| Loktin & Popova | 2017 | 265.08 | -32.254 | â | -0.353 | -4.685 | -9.8 |
| Kharchenko et al. | 2016 | 265.071 | -32.215 | â | â | â | â |
| Dias et al. | 2014 | 265.083 | -32.253 | â | -1.05 | -3.08 | â |
| Kharchenko et al. | 2013 | 265.08 | -32.215 | â | -0.76 | -5.82 | -9.8 |
| Gozha et al. | 2012 | 265.083 | -32.253 | â | â | â | â |
| Piskunov et al. | 2008 | 265.072 | -32.2 | â | â | â | â |
| Kharchenko et al. | 2007 | 265.08 | -32.25 | â | 0.4 | â | -11.5 |
| Piskunov et al. | 2007 | 265.072 | -32.2 | â | â | â | â |
| van den Bergh | 2006 | 265.075 | -32.2 | â | â | â | â |
| Kharchenko et al. | 2005 | 265.08 | -32.2 | â | -1.28 | -5.72 | -11.5 |
| Kharchenko et al. | 2003 | 265.06 | -32.22 | â | 0.22 | -3.39 | â |
| Chen et al. | 2003 | 265.051 | -32.219 | â | -1.57 | -6.61 | 10.4 |
| Dias et al. | 2002 | 265.083 | -32.253 | â | -1.05 | -3.08 | -7.02 |
| Dambis | 1999 | 265.083 | -32.253 | 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 | 0.46 | 0.45 | 0.84 | 80 | 0.101 | 110 | 0.41 | 0.0 |
| Li et al. | 2025 | 0.45 | 0.55 | â | 61 | 0.143 | â | â | â |
| Wei et al. | 2025 | 0.57 | 0.67 | â | 54 | 0.250 | 1025 | 0.41 | â |
| Almeida et al. | 2025 | 0.45 | 0.62 | â | 78 | â | 934 | â | â |
| Alfonso et al. | 2024 | 0.46 | 0.49 | â | 56 | 0.141 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1328(1) | â | â |
| Cavallo et al. | 2024 | 0.48 | 1.55 | â | 23 | -0.420 | â | â | â |
| Hunt & Reffert | 2023 | 0.44 | 0.38 | 0.84 | 52 | â | â | â | â |
| Qin et al. | 2023 | 0.65 | 0.96 | â | 71 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 108 | â | 108 | â | â |
| He et al. | 2022 | â | 0.65 | â | 40 | â | â | â | â |
| Jaehnig et al. | 2021 | 0.46(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 0.45 | 0.43 | â | 93 | â | â | â | 0 |
| Dias et al. | 2021 | 0.45 | 0.62 | â | 78 | 0.142 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.46 | 0.49 | â | 35 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.45 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 48 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.45 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.45 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.49 | 0.45 | â | 94 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.36 | 0.43 | â | 108 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.36 | 0.43 | â | 108 | 0.205 | â | â | â |
| Gozha et al. | 2012 | 0.49 | â | â | 94 | 0.060 | 110 | â | â |
| Piskunov et al. | 2008 | 0.49 | 0.43 | â | 81 | â | 70(1) | â | â |
| Piskunov et al. | 2007 | 0.49 | 0.43 | â | 81 | â | 34 | â | â |
| van den Bergh | 2006 | 0.49 | 0.43 | â | 93 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.49 | 0.43 | â | 81 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.49 | 0.43 | â | â | â | â | â | â |
| Chen et al. | 2003 | 0.49 | 0.45 | â | 90 | 0.060(1) | â | â | â |
| Dias et al. | 2002 | 0.49 | 0.45 | â | 94 | 0.060 | â | â | â |
| Dambis | 1999 | 0.46 | 0.44 | â | 79 | 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. Gold sample.
Cavallo et al. (2024)
Gold sample.