VDBH 84
(vdBergh-Hagen 84; MWSC 1743; BH 84)
0.83
UTI
0.77
CN
1.0
Cdens
0.75
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
1.3 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
VDBH 84 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate 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 well-studied in the literature.
Distant
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 150.33 | -58.218 | 0.224 | -4.856 | 3.316 | 18.383 |
| Hu & Soubiran | 2025 | 150.354 | -58.22 | â | â | â | â |
| Almeida et al. | 2025 | 150.34 | -58.217 | â | â | â | â |
| Hunt & Reffert | 2024 | 150.331 | -58.224 | 0.23 | -4.877 | 3.329 | 18.373 |
| Cavallo et al. | 2024 | 150.354 | -58.22 | 0.228 | â | â | â |
| Hunt & Reffert | 2023 | 150.331 | -58.224 | 0.23 | -4.877 | 3.329 | 18.373 |
| Just et al. | 2023 | 150.331 | -58.212 | â | â | â | â |
| Dias et al. | 2021 | 150.34 | -58.217 | 0.184 | -4.827 | 3.285 | â |
| Cantat-Gaudin et al. | 2020 | 150.331 | -58.218 | 0.2 | -4.848 | 3.289 | â |
| Cantat-Gaudin & Anders | 2020 | 150.331 | -58.218 | 0.2 | -4.848 | 3.289 | â |
| Soubiran et al. | 2018 | 150.331 | -58.218 | â | â | â | 15.58 |
| Cantat-Gaudin et al. | 2018 | 150.331 | -58.218 | 0.2 | -4.848 | 3.289 | â |
| Kharchenko et al. | 2016 | 150.331 | -58.212 | â | â | â | â |
| Dias et al. | 2014 | 150.329 | -58.217 | â | -6.15 | 4.04 | â |
| Kharchenko et al. | 2013 | 150.337 | -58.215 | â | -4.35 | 5.32 | â |
| Dias et al. | 2002 | 150.329 | -58.217 | â | -6.3 | 4.08 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.380* | â | â | â |
| Almeida et al. | 2025 | 2.40 | 1.69 | â | 1125 | â | 428 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1071* | â | â |
| Cavallo et al. | 2024 | 3.63 | 2.58 | â | 603 | 0.300 | â | â | â |
| Hunt & Reffert | 2023 | 3.80 | 2.75 | 2.24 | 161 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 50 | â | 16 | â | â |
| Dias et al. | 2021 | 2.40 | 1.69 | â | 1125 | 0.205 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 4.45 | 2.09 | â | 135 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.38 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 4.38 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.38 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.28 | 1.55 | â | 50 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.28 | 1.55 | â | 50 | â | â | â | â |
| Dias et al. | 2002 | 3.37 | 1.95 | â | 562 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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