Melotte 106

(Collinder 247; NGC 3680; MWSC 1942; OCL 823; ESO 265 32; FSR 1548; FoF 2260)

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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

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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.

Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: good fit.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 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 –
Hu & Soubiran 2025 171.36 -43.252 – – – –
Almeida et al. 2025 171.387 -43.249 – – – –
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 – – –
Hunt & Reffert 2023 171.405 -43.228 0.94 -7.258 1.223 1.985
Almeida et al. 2023 171.428 -43.262 – – – –
Just et al. 2023 171.397 -43.231 – – – –
He et al. 2022 171.405 -43.231 0.946 -7.253 1.223 –
Tarricq et al. 2022 171.364 -43.225 0.957 -7.251 1.246 –
Jaehnig et al. 2021 171.387 -43.228 0.954 -7.284 1.158 –
Rain et al. 2021 171.392 -43.24 0.933 -7.278 1.118 –
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 –
Cantat-Gaudin & Anders 2020 171.392 -43.24 0.933 -7.278 1.118 –
Liu & Pang 2019 171.377 -43.219 0.929 -7.255 1.153 –
Soubiran et al. 2018 171.392 -43.24 – – – 1.74
Bica et al. 2019 171.404 -43.241 – – – –
Cantat-Gaudin et al. 2018 171.392 -43.24 0.933 -7.278 1.118 –
Angelo et al. 2019 171.417 -43.236 – – – –
Loktin & Popova 2017 171.405 -43.243 – -5.42 2.29 2.4
Kharchenko et al. 2016 171.397 -43.231 – – – –
Dias et al. 2014 171.408 -43.243 – -5.42 2.29 –
Kharchenko et al. 2013 171.405 -43.235 – -5.21 0.77 2.4
Gozha et al. 2012 171.408 -43.243 – – – –
Piskunov et al. 2008 171.392 -43.237 – – – –
Kharchenko et al. 2007 171.4 -43.24 – 0.21 – –
Piskunov et al. 2007 171.392 -43.237 – – – –
van den Bergh 2006 171.408 -43.243 – – – –
Kharchenko et al. 2005 171.4 -43.24 – -5.38 1.54 –
Kharchenko et al. 2003 171.42 -43.24 – -5.1 1.41 –
Chen et al. 2003 171.436 -43.26 – -5.3 0.46 0.9
Dias et al. 2002 171.408 -43.243 – -5.42 2.29 1.28

💡 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 99999– 1.0 0.22 0.18 1549 -0.139 122 0.53 1.0
Li et al. 2025 1.04 0.18 – 2006 -0.013 – – –
Hu & Soubiran 2025 – – – – -0.140(5) – – –
Almeida et al. 2025 1.03 0.27 – 1959 – 207 – –
Hunt & Reffert 2024 – – – – – 170(1) – –
Cavallo et al. 2024 1.03 0.36 – 1549 0.160 – – –
Hunt & Reffert 2023 1.00 0.10 0.18 1493 – – – –
Almeida et al. 2023 1.01 0.31 – 2004 -0.137 366(1) 0.53 –
Just et al. 2023 – – – 1585 – 49 – –
He et al. 2022 – 0.25 – 1778 – – – –
Tarricq et al. 2022 1.04 – – 2138 – – – –
Jaehnig et al. 2021 1.04(1) – – – – – – –
Rain et al. 2021 1.04 0.19 – 1175 – – – 1
Dias et al. 2021 1.03 0.27 – 1959 -0.041 – – –
Cantat-Gaudin et al. 2020 1.07 0.10 – 2188 – – – –
Cantat-Gaudin & Anders 2020 1.04 – – – – – – –
Liu & Pang 2019 – – – 269 -0.750 – – –
Soubiran et al. 2018 1.04 – – – – – – –
Cantat-Gaudin et al. 2018 1.04 – – – – – – –
Angelo et al. 2019 0.95 – – 1580 – 102 – –
Loktin & Popova 2017 0.93 0.21 – 1309 – – – –
Kharchenko et al. 2016 0.95 0.19 – 1585 – – – –
Kharchenko et al. 2013 0.95 0.19 – 1585 -0.167 – – –
Gozha et al. 2012 0.94 – – 1194 -0.190 110 – –
Piskunov et al. 2008 0.93 0.22 – 1230 – 133(1) – –
Piskunov et al. 2007 0.93 0.22 – 1230 – 50 – –
van den Bergh 2006 0.94 0.22 – 1202 – – – –
Kharchenko et al. 2005 0.93 0.22 – 1230 – – – –
Kharchenko et al. 2003 0.94 0.22 – – – – – –
Chen et al. 2003 0.94 0.20 – 1190 -0.090(1) – – –
Dias et al. 2002 0.94 0.20 – 1194 -0.190 – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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