Melotte 106
(Collinder 247; NGC 3680; MWSC 1942; OCL 823; ESO 265 32; FSR 1548; FoF 2260)
0.94
UTI
0.72
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
15.3 [N/pc2]
- CN 0.72 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Melotte 106 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (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 | 99999â | 171.395 | -43.237 | 0.945 | -7.263 | 1.197 | 2.045 |
| Li et al. | 2025 | 171.392 | -43.24 | 0.933 | -7.278 | 1.118 | â |
| Hu & Soubiran | 2025 | 171.36 | -43.252 | â | â | â | â |
| Almeida et al. | 2025 | 171.387 | -43.249 | â | â | â | â |
| Hunt & Reffert | 2024 | 171.405 | -43.228 | 0.94 | -7.258 | 1.223 | 1.985 |
| Cavallo et al. | 2024 | 171.36 | -43.251 | 0.944 | â | â | â |
| Hunt & Reffert | 2023 | 171.405 | -43.228 | 0.94 | -7.258 | 1.223 | 1.985 |
| Almeida et al. | 2023 | 171.428 | -43.262 | â | â | â | â |
| Just et al. | 2023 | 171.397 | -43.231 | â | â | â | â |
| He et al. | 2022 | 171.405 | -43.231 | 0.946 | -7.253 | 1.223 | â |
| Tarricq et al. | 2022 | 171.364 | -43.225 | 0.957 | -7.251 | 1.246 | â |
| Jaehnig et al. | 2021 | 171.387 | -43.228 | 0.954 | -7.284 | 1.158 | â |
| Rain et al. | 2021 | 171.392 | -43.24 | 0.933 | -7.278 | 1.118 | â |
| Dias et al. | 2021 | 171.387 | -43.249 | 0.934 | -7.271 | 1.131 | 2.922 |
| Cantat-Gaudin et al. | 2020 | 171.392 | -43.24 | 0.933 | -7.278 | 1.118 | â |
| Cantat-Gaudin & Anders | 2020 | 171.392 | -43.24 | 0.933 | -7.278 | 1.118 | â |
| Liu & Pang | 2019 | 171.377 | -43.219 | 0.929 | -7.255 | 1.153 | â |
| Soubiran et al. | 2018 | 171.392 | -43.24 | â | â | â | 1.74 |
| Bica et al. | 2019 | 171.404 | -43.241 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 171.392 | -43.24 | 0.933 | -7.278 | 1.118 | â |
| Angelo et al. | 2019 | 171.417 | -43.236 | â | â | â | â |
| Loktin & Popova | 2017 | 171.405 | -43.243 | â | -5.42 | 2.29 | 2.4 |
| Kharchenko et al. | 2016 | 171.397 | -43.231 | â | â | â | â |
| Dias et al. | 2014 | 171.408 | -43.243 | â | -5.42 | 2.29 | â |
| Kharchenko et al. | 2013 | 171.405 | -43.235 | â | -5.21 | 0.77 | 2.4 |
| Gozha et al. | 2012 | 171.408 | -43.243 | â | â | â | â |
| Piskunov et al. | 2008 | 171.392 | -43.237 | â | â | â | â |
| Kharchenko et al. | 2007 | 171.4 | -43.24 | â | 0.21 | â | â |
| Piskunov et al. | 2007 | 171.392 | -43.237 | â | â | â | â |
| van den Bergh | 2006 | 171.408 | -43.243 | â | â | â | â |
| Kharchenko et al. | 2005 | 171.4 | -43.24 | â | -5.38 | 1.54 | â |
| Kharchenko et al. | 2003 | 171.42 | -43.24 | â | -5.1 | 1.41 | â |
| Chen et al. | 2003 | 171.436 | -43.26 | â | -5.3 | 0.46 | 0.9 |
| Dias et al. | 2002 | 171.408 | -43.243 | â | -5.42 | 2.29 | 1.28 |
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 | 1.0 | 0.22 | 0.18 | 1549 | -0.139 | 122 | 0.53 | 1.0 |
| Li et al. | 2025 | 1.04 | 0.18 | â | 2006 | -0.013 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.140(5) | â | â | â |
| Almeida et al. | 2025 | 1.03 | 0.27 | â | 1959 | â | 207 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 170(1) | â | â |
| Cavallo et al. | 2024 | 1.03 | 0.36 | â | 1549 | 0.160 | â | â | â |
| Hunt & Reffert | 2023 | 1.00 | 0.10 | 0.18 | 1493 | â | â | â | â |
| Almeida et al. | 2023 | 1.01 | 0.31 | â | 2004 | -0.137 | 366(1) | 0.53 | â |
| Just et al. | 2023 | â | â | â | 1585 | â | 49 | â | â |
| He et al. | 2022 | â | 0.25 | â | 1778 | â | â | â | â |
| Tarricq et al. | 2022 | 1.04 | â | â | 2138 | â | â | â | â |
| Jaehnig et al. | 2021 | 1.04(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 1.04 | 0.19 | â | 1175 | â | â | â | 1 |
| Dias et al. | 2021 | 1.03 | 0.27 | â | 1959 | -0.041 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.07 | 0.10 | â | 2188 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.04 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 269 | -0.750 | â | â | â |
| Soubiran et al. | 2018 | 1.04 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.04 | â | â | â | â | â | â | â |
| Angelo et al. | 2019 | 0.95 | â | â | 1580 | â | 102 | â | â |
| Loktin & Popova | 2017 | 0.93 | 0.21 | â | 1309 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.95 | 0.19 | â | 1585 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.95 | 0.19 | â | 1585 | -0.167 | â | â | â |
| Gozha et al. | 2012 | 0.94 | â | â | 1194 | -0.190 | 110 | â | â |
| Piskunov et al. | 2008 | 0.93 | 0.22 | â | 1230 | â | 133(1) | â | â |
| Piskunov et al. | 2007 | 0.93 | 0.22 | â | 1230 | â | 50 | â | â |
| van den Bergh | 2006 | 0.94 | 0.22 | â | 1202 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.93 | 0.22 | â | 1230 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.94 | 0.22 | â | â | â | â | â | â |
| Chen et al. | 2003 | 0.94 | 0.20 | â | 1190 | -0.090(1) | â | â | â |
| Dias et al. | 2002 | 0.94 | 0.20 | â | 1194 | -0.190 | 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: worst fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.