Lynga 2

(FoF 2308)

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C3
N_50
r_50
AA 191 9.1
Summary

Lynga 2 is a rich, very dense object of very high C3 quality. It is located at a close distance from the Sun, near the mid-plane. It is very well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 216.146 -61.331 -5.26 -5.42 -9.94
Piskunov et al. (2007) 216.088 -61.328
Piskunov et al. (2008) 216.088 -61.328
Kharchenko et al. (2012) 216.113 -61.33 -6.25 -6.5
Loktin & Popova (2017) 216.15 -61.332 -4.738 -8.163 -9.9
Cantat-Gaudin et al. (2018) 216.085 -61.328 1.034 -6.716 -4.696
Soubiran et al. (2018) 216.085 -61.328 -12.35
Bossini et al. (2019) 216.085 -61.328
Liu & Pang (2019) 216.061 -61.333 1.036 -6.663 -4.703
Cantat-Gaudin et al. (2020) 216.085 -61.328 1.034 -6.716 -4.696
Dias et al. (2021) 216.081 -61.333 1.034 -6.71 -4.682
Rain et al. (2021) 216.085 -61.328 1.034 -6.716 -4.696
Jaehnig et al. (2021) 216.098 -61.325 1.061 -6.7 -4.688
Tarricq et al. (2022) 216.046 -61.325 1.042 -6.751 -4.668
He et al. (2022) 216.084 -61.332 1.048 -6.752 -4.655
Cordoni et al. (2023) 216.081 -61.333 1.034 -6.71 -4.682
Hunt & Reffert (2023) 216.057 -61.333 1.047 -6.749 -4.663 -18.022
Cavallo et al. (2024) 216.062 -61.334 1.053
Hunt & Reffert (2024) 216.057 -61.333 1.047 -6.749 -4.663 -18.022
Alfonso et al. (2024) 216.046 -61.33 1.013 -6.748 -4.655
Almeida et al. (2025) 216.081 -61.333
           
UCC 216.075 -61.325 1.047 -6.762 -4.663 -17.471
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Explore data in Colab

Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.22, Dist=900.0, Age=7.95
Piskunov et al. (2007) E(B-V)=0.2, Dist=1000, logt=8.42, logM=1.559
Piskunov et al. (2008) E(B-V)=0.2, Dist=1000, logt=8.42, logM=2.227, logMA=2.203
Kharchenko et al. (2012) e_bv=0.323, distance=932, log_age=8.43
Loktin & Popova (2017) E(B-V)=0.217, Dist=1032, logt=8.163
Cantat-Gaudin et al. (2018) dmode=940.4
Soubiran et al. (2018) dmode=940.4
Bossini et al. (2019) AV=0.691, Dist=9.862, logA=7.933, Fe/H=0.0
Liu & Pang (2019) Age=0.093, Z=0.25
Cantat-Gaudin et al. (2020) AVNN=0.79, DistPc=970.0, AgeNN=8.01
Dias et al. (2021) Av=0.973, Dist=922, logage=8.208, [Fe/H]=0.046
Rain et al. (2021) E(B-V)=0.22, Dist=940.4, log(Age)=7.93, NBSS=0
Jaehnig et al. (2021) dmode=0.94
Tarricq et al. (2022) Dist=946, logAgeNN=8.03
He et al. (2022) A0=1.05, logAge=7.85
Cordoni et al. (2023) Av=0.973, Dist=9.824, logAge=8.208, [Fe/H]=0.046, mass-single=521.616, fbin-tot=0.246, fbss-MS=0.0
Hunt & Reffert (2023) AV50=0.734, diffAV50=0.726, MOD50=9.768, logAge50=8.044
Cavallo et al. (2024) AV50=0.77, dMod50=9.8, logAge50=8.33, [Fe/H]50=0.33
Hunt & Reffert (2024) MassJ=534.745, MassTot=534.745
Alfonso et al. (2024) AV=0.78902, MOD=9.93049, logAge=7.98524, Z=0.04548
Almeida et al. (2025) AV=0.973, Dist=922, logAge=8.208, MassRk=433.6

Search coordinates in Bayestar19

Cluster region map