Lynga 2

(MWSC 2215; FoF 2308)

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0.96 UTI
0.78
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad) 29.9 [N/pc2]
  • CN 0.78 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

ℹ️
Lynga 2 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.

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

Cavallo et al. (2024)
Gold sample.

Data

ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 216.075 -61.325 1.047 -6.762 -4.663 -17.471
Li et al. 2025 216.085 -61.328 1.034 -6.716 -4.696 –
Wei et al. 2025 216.096 -61.337 1.055 -6.678 -4.648 –
Almeida et al. 2025 216.081 -61.333 – – – –
Alfonso et al. 2024 216.046 -61.33 1.013 -6.748 -4.655 –
Hunt & Reffert 2024 216.057 -61.333 1.047 -6.749 -4.663 -18.022
Cavallo et al. 2024 216.062 -61.334 1.053 – – –
Hunt & Reffert 2023 216.057 -61.333 1.047 -6.749 -4.663 -18.022
Almeida et al. 2023 216.166 -61.354 – – – –
Cordoni et al. 2023 216.081 -61.333 1.034 -6.71 -4.682 –
Just et al. 2023 216.1 -61.327 – – – –
He et al. 2022 216.084 -61.332 1.048 -6.752 -4.655 –
Tarricq et al. 2022 216.046 -61.325 1.042 -6.751 -4.668 –
Jaehnig et al. 2021 216.098 -61.325 1.061 -6.7 -4.688 –
Rain et al. 2021 216.085 -61.328 1.034 -6.716 -4.696 –
Dias et al. 2021 216.081 -61.333 1.034 -6.71 -4.682 –
Cantat-Gaudin et al. 2020 216.085 -61.328 1.034 -6.716 -4.696 –
SΓ‘nchez et al. 2020 216.146 -61.331 – -6.665 -4.559 –
Cantat-Gaudin & Anders 2020 216.085 -61.328 1.034 -6.716 -4.696 –
Liu & Pang 2019 216.061 -61.333 1.036 -6.663 -4.703 –
Bossini et al. 2019 216.085 -61.328 – – – –
Soubiran et al. 2018 216.085 -61.328 – – – -12.35
Cantat-Gaudin et al. 2018 216.085 -61.328 1.034 -6.716 -4.696 –
Loktin & Popova 2017 216.15 -61.332 – -4.738 -8.163 -9.9
Kharchenko et al. 2016 216.1 -61.327 – – – –
Dias et al. 2014 216.146 -61.331 – -5.26 -5.42 –
Kharchenko et al. 2013 216.112 -61.33 – -6.25 -6.5 -9.9
Gozha et al. 2012 216.146 -61.331 – – – –
Piskunov et al. 2008 216.088 -61.328 – – – –
Piskunov et al. 2007 216.088 -61.328 – – – –
van den Bergh 2006 216.088 -61.322 – – – –
Kharchenko et al. 2005 216.09 -61.33 – -5.45 -7.6 –
Kharchenko et al. 2003 216.04 -61.35 – -5.25 -6.27 –
Dias et al. 2002 216.146 -61.331 – -5.26 -5.42 -9.94

πŸ’‘ 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– 0.94 0.78 0.73 132 0.046 367 0.29 0.0
Li et al. 2025 0.87 0.92 – 151 -0.153 – – –
Wei et al. 2025 1.35 0.87 – 95 0.500 632 0.29 –
Almeida et al. 2025 0.92 0.97 – 161 – 434 – –
Alfonso et al. 2024 0.97 0.79 – 97 0.045 – – –
Hunt & Reffert 2024 – – – – – 535(1) – –
Cavallo et al. 2024 0.91 0.77 – 214 0.330 – – –
Hunt & Reffert 2023 0.90 0.73 0.73 111 – – – –
Almeida et al. 2023 0.92 1.03 – 112 -0.050 367(1) 0.44 –
Cordoni et al. 2023 0.92 0.97 – 161 0.046 522 0.25 0.00
Just et al. 2023 – – – 269 – 75 – –
He et al. 2022 – 1.05 – 71 – – – –
Tarricq et al. 2022 0.95 – – 107 – – – –
Jaehnig et al. 2021 0.94(1) – – – – – – –
Rain et al. 2021 0.94 0.68 – 85 – – – 0
Dias et al. 2021 0.92 0.97 – 161 0.046 – – –
Cantat-Gaudin et al. 2020 0.97 0.79 – 102 – – – –
Cantat-Gaudin & Anders 2020 0.94 – – – – – – –
Liu & Pang 2019 – – – 93 0.250 – – –
Bossini et al. 2019 0.94 0.69 – 86 0.000 – – –
Soubiran et al. 2018 0.94 – – – – – – –
Cantat-Gaudin et al. 2018 0.94 – – – – – – –
Loktin & Popova 2017 1.03 0.67 – 146 – – – –
Kharchenko et al. 2016 0.93 1.00 – 269 – – – –
Kharchenko et al. 2013 0.93 1.00 – 269 – – – –
Gozha et al. 2012 0.90 – – 89 – 158 – –
Piskunov et al. 2008 1.00 0.62 – 263 – 169(1) – –
Piskunov et al. 2007 1.00 0.62 – 263 – 36 – –
van den Bergh 2006 1.00 0.62 – 132 – – – –
Kharchenko et al. 2005 1.00 0.62 – 263 – – – –
Kharchenko et al. 2003 1.00 0.62 – – – – – –
Dias et al. 2002 0.90 0.68 – 89 – – – –

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

Visualization

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