VDBH 88
(vdBergh-Hagen 88; MWSC 1764; BH 88)
0.66
UTI
0.27
CN
1.0
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
2.8 [arcmin]
- CN 0.27 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
VDBH 88 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above 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 mass parameter (see Parameters). It is moderately studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Relatively close
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 | 151.616 | -51.551 | 0.515 | -6.195 | 3.64 | 6.824 |
| Almeida et al. | 2025 | 151.621 | -51.556 | â | â | â | â |
| Hunt & Reffert | 2024 | 151.615 | -51.555 | 0.534 | -6.18 | 3.638 | 22.364 |
| Cavallo et al. | 2024 | 151.574 | -51.526 | 0.538 | â | â | â |
| Hunt & Reffert | 2023 | 151.615 | -51.555 | 0.534 | -6.18 | 3.638 | 22.364 |
| Just et al. | 2023 | 151.561 | -51.592 | â | â | â | â |
| Dias et al. | 2021 | 151.621 | -51.556 | 0.386 | -6.086 | 3.602 | 22.751 |
| Bica et al. | 2019 | 151.575 | -51.61 | â | â | â | â |
| Kharchenko et al. | 2016 | 151.561 | -51.592 | â | â | â | â |
| Dias et al. | 2014 | 151.625 | -51.567 | â | -4.82 | 3.94 | â |
| Kharchenko et al. | 2013 | 151.567 | -51.595 | â | -9.15 | 8.65 | â |
| Dias et al. | 2002 | 151.625 | -51.567 | â | -4.82 | 3.94 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 2.01 | 1.61 | â | 583 | â | 158 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 135* | â | â |
| Cavallo et al. | 2024 | 1.83 | 1.44 | â | 380 | 0.410 | â | â | â |
| Hunt & Reffert | 2023 | 1.77 | 1.44 | 1.01 | 472 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1259 | â | 6012 | â | â |
| Dias et al. | 2021 | 2.01 | 1.61 | â | 583 | -0.141 | â | â | â |
| Kharchenko et al. | 2016 | 5.82 | 1.68 | â | 1259 | â | â | â | â |
| Kharchenko et al. | 2013 | 5.82 | 1.68 | â | 1259 | â | â | â | â |
| Dias et al. | 2002 | 1.77 | 1.86 | â | 126 | 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: good fit.
Cavallo et al. (2024)
Gold sample.