VDBH 55
(vdBergh-Hagen 55; MWSC 1600; BH 55; ESO 314 01; FSR 1404)
0.86
UTI
0.8
CN
1.0
Cdens
0.75
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
3.0 [arcmin]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
VDBH 55 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is well-studied in the literature.
Distant
Moderate extinction
Massive
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 134.04 | -39.517 | 0.213 | -3.935 | 3.136 | 32.809 |
| Hu & Soubiran | 2025 | 134.03 | -39.503 | â | â | â | â |
| Almeida et al. | 2025 | 134.043 | -39.516 | â | â | â | â |
| Hunt & Reffert | 2024 | 134.041 | -39.522 | 0.223 | -3.93 | 3.126 | 38.761 |
| Cavallo et al. | 2024 | 134.03 | -39.503 | 0.218 | â | â | â |
| Hunt & Reffert | 2023 | 134.041 | -39.522 | 0.223 | -3.93 | 3.126 | 38.761 |
| Just et al. | 2023 | 134.042 | -39.507 | â | â | â | â |
| Dias et al. | 2021 | 134.043 | -39.516 | 0.188 | -3.992 | 3.14 | 32.779 |
| Cantat-Gaudin et al. | 2020 | 134.042 | -39.518 | 0.185 | -3.971 | 3.118 | â |
| Cantat-Gaudin & Anders | 2020 | 134.042 | -39.518 | 0.185 | -3.971 | 3.118 | â |
| Soubiran et al. | 2018 | 134.042 | -39.518 | â | â | â | 35.15 |
| Bica et al. | 2019 | 134.031 | -39.517 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 134.042 | -39.518 | 0.185 | -3.971 | 3.118 | â |
| Kharchenko et al. | 2016 | 134.042 | -39.507 | â | â | â | â |
| Dias et al. | 2014 | 134.046 | -39.517 | â | -2.09 | 1.87 | â |
| Kharchenko et al. | 2013 | 134.047 | -39.51 | â | -5.28 | 6.55 | â |
| Dias et al. | 2002 | 134.046 | -39.517 | â | -4.9 | 6.97 | 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 | -0.080* | â | â | â |
| Almeida et al. | 2025 | 4.64 | 1.79 | â | 2483 | â | 1037 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1138* | â | â |
| Cavallo et al. | 2024 | 3.33 | 2.20 | â | 1318 | -0.410 | â | â | â |
| Hunt & Reffert | 2023 | 4.04 | 2.02 | 2.24 | 587 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 28 | â | 1285 | â | â |
| Dias et al. | 2021 | 4.64 | 1.79 | â | 2483 | -0.125 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 4.79 | 1.22 | â | 2291 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.67 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 4.67 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.67 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 3.64 | 6.68 | â | 28 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.64 | 6.68 | â | 28 | â | â | â | â |
| Dias et al. | 2002 | 4.11 | 1.30 | â | 1122 | 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.