Collinder 132
Summary
Collinder 132 is a sparse, loose object of high C3 quality. It is located at a close distance from the Sun, below the mid-plane. It is very well-studied in the literature.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 108.833 | -30.683 | – | -2.01 | 2.9 | 26.58 |
| Piskunov et al. (2008) | 108.385 | -31.028 | – | – | – | – |
| Kharchenko et al. (2012) | 108.36 | -30.975 | – | -5.3 | 4.71 | – |
| Loktin & Popova (2017) | 108.84 | -30.682 | – | -1.685 | 3.679 | 28.0 |
| Cantat-Gaudin et al. (2018) | 108.485 | -30.758 | 1.501 | -4.14 | 3.732 | – |
| Soubiran et al. (2018) | 108.485 | -30.758 | – | – | – | 24.13 |
| Dias et al. (2019) | 108.483 | -30.758 | 1.501 | -4.14 | 3.732 | 27.339 |
| Cantat-Gaudin et al. (2020) | 108.485 | -30.758 | 1.501 | -4.14 | 3.732 | – |
| Dias et al. (2021) | 108.595 | -30.703 | 1.5 | -4.128 | 3.687 | 36.91 |
| Rain et al. (2021) | 108.485 | -30.758 | 1.501 | -4.14 | 3.732 | – |
| Jaehnig et al. (2021) | 108.79 | -30.672 | 1.49 | -4.067 | 3.547 | – |
| Hunt & Reffert (2023) | 108.346 | -30.971 | 1.525 | -4.125 | 3.727 | 18.565 |
| Cavallo et al. (2024) | 108.549 | -30.822 | 1.529 | – | – | – |
| Celli et al. (2024) | 108.485 | -30.758 | – | – | – | – |
| Hunt & Reffert (2024) | 108.346 | -30.971 | 1.525 | -4.125 | 3.727 | 18.565 |
| Alfonso et al. (2024) | 108.752 | -31.126 | 1.485 | -4.146 | 3.711 | – |
| Almeida et al. (2025) | 108.595 | -30.703 | – | – | – | – |
| UCC | 108.367 | -30.922 | 1.541 | -4.119 | 3.769 | 17.973 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.037, Dist=472.0, Age=7.08 |
| Piskunov et al. (2008) | E(B-V)=0.02, Dist=411, logt=7.51, logMA=1.182 |
| Kharchenko et al. (2012) | e_bv=0.021, distance=330, log_age=7.51 |
| Loktin & Popova (2017) | E(B-V)=0.029, Dist=425, logt=7.049 |
| Cantat-Gaudin et al. (2018) | dmode=653.5 |
| Soubiran et al. (2018) | dmode=653.5 |
| Dias et al. (2019) | E(B-V)=0.05, Dist=660, logAge=7.668, Z=0.015 |
| Cantat-Gaudin et al. (2020) | AVNN=0.0, DistPc=624.0, AgeNN=7.39 |
| Dias et al. (2021) | Av=0.199, Dist=648, logage=7.488, [Fe/H]=0.037 |
| Rain et al. (2021) | E(B-V)=0.03, Dist=653.5, log(Age)=7.08, NBSS=0 |
| Jaehnig et al. (2021) | dmode=0.709 |
| Hunt & Reffert (2023) | AV50=0.123, diffAV50=0.518, MOD50=9.0, logAge50=7.142 |
| Cavallo et al. (2024) | AV50=0.46, dMod50=9.14, logAge50=6.91, [Fe/H]50=-0.29 |
| Celli et al. (2024) | Age=24.5, Mc=196.2 |
| Hunt & Reffert (2024) | MassJ=48.7521, MassTot=132.498 |
| Alfonso et al. (2024) | AV=0.00073, MOD=8.97975, logAge=7.39474, Z=0.0371 |
| Almeida et al. (2025) | AV=0.199, Dist=648, logAge=7.488, MassRk=195.3 |
Search coordinates in Bayestar19