VDBH 132
(vdBergh-Hagen 132; MWSC 2032; BH 132)
0.87
UTI
0.74
CN
1.0
Cdens
1.0
CC3
0.81
Clit
1.0
Cdup
Stellar density (N50/rad)
24.9 [N/pc2]
- CN 0.74 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
VDBH 132 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 186.738 | -64.058 | 0.368 | -6.255 | -0.187 | -19.521 |
| Almeida et al. | 2025 | 186.725 | -64.064 | â | â | â | â |
| Hunt & Reffert | 2024 | 186.731 | -64.056 | 0.374 | -6.243 | -0.192 | -23.256 |
| Cavallo et al. | 2024 | 186.736 | -64.056 | 0.373 | â | â | â |
| Hunt & Reffert | 2023 | 186.731 | -64.056 | 0.374 | -6.243 | -0.192 | -23.256 |
| Just et al. | 2023 | 186.74 | -64.064 | â | â | â | â |
| Dias et al. | 2021 | 186.725 | -64.064 | 0.367 | -6.222 | -0.179 | â |
| Cantat-Gaudin et al. | 2020 | 186.72 | -64.058 | 0.362 | -6.22 | -0.177 | â |
| Cantat-Gaudin & Anders | 2020 | 186.72 | -64.058 | 0.362 | -6.22 | -0.177 | â |
| Soubiran et al. | 2018 | 186.72 | -64.058 | â | â | â | -18.94 |
| Bica et al. | 2019 | 186.747 | -64.045 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 186.72 | -64.058 | 0.362 | -6.22 | -0.177 | â |
| Kharchenko et al. | 2016 | 186.74 | -64.064 | â | â | â | â |
| Dias et al. | 2014 | 186.75 | -64.067 | â | -4.45 | -0.95 | â |
| Kharchenko et al. | 2013 | 186.75 | -64.067 | â | -8.07 | 2.9 | â |
| Dias et al. | 2002 | 186.75 | -64.067 | â | -4.45 | -0.95 | â |
đĄ 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 | 99999â | 2.42 | 1.59 | 2.52 | 282 | 0.207 | 406 | â | â |
| Almeida et al. | 2025 | 2.17 | 1.59 | â | 132 | â | 406 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 977(1) | â | â |
| Cavallo et al. | 2024 | 2.22 | 1.66 | â | 309 | 0.130 | â | â | â |
| Hunt & Reffert | 2023 | 2.42 | 1.75 | 2.52 | 95 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 282 | â | 387 | â | â |
| Dias et al. | 2021 | 2.17 | 1.59 | â | 132 | 0.285 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.55 | 1.24 | â | 158 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.56 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.56 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.56 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.86 | 1.48 | â | 282 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.86 | 1.48 | â | 282 | â | â | â | â |
| Dias et al. | 2002 | 5.23 | 2.00 | â | 2512 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.