VDBH 132
(vdBergh-Hagen 132; BH 132; MWSC 2032)
Summary
VDBH 132 is a moderately populated, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is well-studied in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 186.75 | -64.067 | – | -4.45 | -0.95 | – |
| Kharchenko et al. (2012) | 186.75 | -64.067 | – | -8.07 | 2.9 | – |
| Cantat-Gaudin et al. (2018) | 186.72 | -64.058 | 0.362 | -6.22 | -0.177 | – |
| Bica et al. (2019) | 186.747 | -64.045 | – | – | – | – |
| Soubiran et al. (2018) | 186.72 | -64.058 | – | – | – | -18.94 |
| Cantat-Gaudin et al. (2020) | 186.72 | -64.058 | 0.362 | -6.22 | -0.177 | – |
| Dias et al. (2021) | 186.725 | -64.064 | 0.367 | -6.222 | -0.179 | – |
| Hunt & Reffert (2023) | 186.731 | -64.056 | 0.374 | -6.243 | -0.192 | -23.256 |
| Cavallo et al. (2024) | 186.736 | -64.056 | 0.373 | – | – | – |
| Hunt & Reffert (2024) | 186.731 | -64.056 | 0.374 | -6.243 | -0.192 | -23.256 |
| Almeida et al. (2025) | 186.725 | -64.064 | – | – | – | – |
| UCC | 186.738 | -64.058 | 0.368 | -6.255 | -0.187 | -19.521 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.645, Dist=5229.0, Age=9.4 |
| Kharchenko et al. (2012) | e_bv=0.479, distance=1859, log_age=8.45 |
| Cantat-Gaudin et al. (2018) | dmode=2557.8 |
| Soubiran et al. (2018) | dmode=2557.8 |
| Cantat-Gaudin et al. (2020) | AVNN=1.24, DistPc=2541.0, AgeNN=8.2 |
| Dias et al. (2021) | Av=1.589, Dist=2174, logage=8.12, [Fe/H]=0.285 |
| Hunt & Reffert (2023) | AV50=1.746, diffAV50=2.521, MOD50=11.921, logAge50=7.979 |
| Cavallo et al. (2024) | AV50=1.66, dMod50=11.73, logAge50=8.49, [Fe/H]50=0.13 |
| Hunt & Reffert (2024) | MassJ=976.879, MassTot=979.438 |
| Almeida et al. (2025) | AV=1.589, Dist=2174, logAge=8.12, MassRk=406.0 |
Search coordinates in Bayestar19