VDBH 19
(BH 19; vdBergh-Hagen 19; ESO 430 21; MWSC 1433)
0.82
UTI
0.77
CN
1.0
Cdens
0.75
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
2.4 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
VDBH 19 is a rich, very dense object of 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, but with a large variance across recent sources for the age parameter (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 | β | 121.765 | -32.357 | 0.205 | -2.866 | 3.583 | 86.077 |
| Li et al. | 2025 | 121.768 | -32.355 | 0.19 | -2.897 | 3.547 | β |
| Almeida et al. | 2025 | 121.763 | -32.351 | β | β | β | β |
| Hunt & Reffert | 2024 | 121.768 | -32.358 | 0.216 | -2.855 | 3.588 | 86.596 |
| Cavallo et al. | 2024 | 121.756 | -32.359 | 0.211 | β | β | β |
| Hunt & Reffert | 2023 | 121.768 | -32.358 | 0.216 | -2.855 | 3.588 | 86.596 |
| Dias et al. | 2021 | 121.763 | -32.351 | 0.205 | -2.89 | 3.543 | 86.852 |
| Cantat-Gaudin et al. | 2020 | 121.768 | -32.355 | 0.19 | -2.897 | 3.547 | β |
| SΓ‘nchez et al. | 2020 | 121.771 | -32.35 | β | -2.917 | 3.663 | β |
| Cantat-Gaudin & Anders | 2020 | 121.768 | -32.355 | 0.19 | -2.897 | 3.547 | β |
| Soubiran et al. | 2018 | 121.768 | -32.355 | β | β | β | 86.49 |
| Bica et al. | 2019 | 121.77 | -32.352 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 121.768 | -32.355 | 0.19 | -2.897 | 3.547 | β |
| Dias et al. | 2014 | 121.771 | -32.35 | β | -3.48 | -0.83 | β |
| Dias et al. | 2002 | 121.771 | -32.35 | β | -3.48 | -0.83 | β |
π‘ 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 3.94 | 2.58 | β | 279 | -0.047 | β | β | β |
| Almeida et al. | 2025 | 3.62 | 2.43 | β | 326 | β | 404 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 1167* | β | β |
| Cavallo et al. | 2024 | 4.47 | 2.89 | β | 95 | -0.200 | β | β | β |
| Hunt & Reffert | 2023 | 4.10 | 2.34 | 1.97 | 348 | β | β | β | β |
| Dias et al. | 2021 | 3.62 | 2.43 | β | 326 | -0.100 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 4.57 | 1.96 | β | 309 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 4.56 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 4.56 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 4.56 | β | β | β | β | β | β | β |
| Dias et al. | 2002 | 3.05 | 2.20 | β | 282 | β | β | β | β |
(*): 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.