VDBH 78
(vdBergh-Hagen 78; MWSC 1706; BH 78; FSR 1512)
0.82
UTI
0.69
CN
1.0
Cdens
0.75
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
0.8 [arcmin]
- CN 0.69 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
VDBH 78 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~8.29 kpc) differs significantly from the median photometric distance (~5.58 kpc).
Very distant
High 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 | 145.953 | -56.576 | 0.121 | -3.754 | 2.767 | 26.479 |
| Almeida et al. | 2025 | 145.954 | -56.571 | â | â | â | â |
| Hunt & Reffert | 2024 | 145.951 | -56.574 | 0.115 | -3.754 | 2.786 | 26.52 |
| Cavallo et al. | 2024 | 145.962 | -56.579 | 0.114 | â | â | â |
| Hunt & Reffert | 2023 | 145.951 | -56.574 | 0.115 | -3.754 | 2.786 | 26.52 |
| Just et al. | 2023 | 145.946 | -56.562 | â | â | â | â |
| Dias et al. | 2021 | 145.954 | -56.571 | 0.142 | -3.651 | 2.748 | â |
| Cantat-Gaudin et al. | 2020 | 145.952 | -56.574 | 0.15 | -3.69 | 2.71 | â |
| Cantat-Gaudin & Anders | 2020 | 145.952 | -56.574 | 0.15 | -3.69 | 2.71 | â |
| Soubiran et al. | 2018 | 145.952 | -56.574 | â | â | â | 22.37 |
| Bica et al. | 2019 | 145.952 | -56.58 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 145.952 | -56.574 | 0.15 | -3.69 | 2.71 | â |
| Kharchenko et al. | 2016 | 145.946 | -56.562 | â | â | â | â |
| Dias et al. | 2014 | 145.925 | -56.55 | â | 0.13 | 1.3 | â |
| Kharchenko et al. | 2013 | 145.95 | -56.565 | â | -3.44 | 3.16 | â |
| Dias et al. | 2002 | 145.925 | -56.55 | â | 0.13 | 1.3 | 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 | 5.60 | 3.01 | â | 589 | â | 898 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1521* | â | â |
| Cavallo et al. | 2024 | 5.06 | 3.30 | â | 479 | -0.050 | â | â | â |
| Hunt & Reffert | 2023 | 6.90 | 3.73 | 1.72 | 170 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 398 | â | 276 | â | â |
| Dias et al. | 2021 | 5.60 | 3.01 | â | 589 | 0.147 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 5.40 | 3.15 | â | 339 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 5.58 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 5.58 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 5.58 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 9.76 | 3.87 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2013 | 9.76 | 3.87 | â | 398 | â | â | â | â |
| Dias et al. | 2002 | 4.60 | 3.10 | â | 398 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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