VDBH 118
(vdBergh-Hagen 118; MWSC 1939; BH 118; ESO 129 20)
0.84
UTI
0.8
CN
1.0
Cdens
0.75
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
1.0 [arcmin]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
VDBH 118 is a rich, very dense object of high C3 quality. Its parallax locates it at a very large 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 metallicity parameter (see Parameters). It is well-studied in the literature.
Very 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 | β | 170.763 | -58.548 | 0.098 | -4.441 | 1.484 | 3.495 |
| Li et al. | 2025 | 170.765 | -58.549 | 0.065 | -4.406 | 1.45 | β |
| Hu & Soubiran | 2025 | 170.741 | -58.554 | β | β | β | β |
| Hunt & Reffert | 2024 | 170.757 | -58.546 | 0.106 | -4.462 | 1.499 | 23.298 |
| Cavallo et al. | 2024 | 170.741 | -58.554 | 0.104 | β | β | β |
| Hunt & Reffert | 2023 | 170.757 | -58.546 | 0.106 | -4.462 | 1.499 | 23.298 |
| Just et al. | 2023 | 170.618 | -58.526 | β | β | β | β |
| Cantat-Gaudin et al. | 2020 | 170.765 | -58.549 | 0.065 | -4.406 | 1.45 | β |
| SΓ‘nchez et al. | 2020 | 170.762 | -58.55 | β | -4.322 | 1.25 | β |
| Cantat-Gaudin & Anders | 2020 | 170.765 | -58.549 | 0.065 | -4.406 | 1.45 | β |
| Bica et al. | 2019 | 170.754 | -58.553 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 170.765 | -58.549 | 0.065 | -4.406 | 1.45 | β |
| Kharchenko et al. | 2016 | 170.618 | -58.526 | β | β | β | β |
| Dias et al. | 2014 | 170.762 | -58.55 | β | -5.47 | -3.06 | β |
| Kharchenko et al. | 2013 | 170.625 | -58.53 | β | -8.23 | 1.23 | β |
| Dias et al. | 2002 | 170.762 | -58.55 | β | -7.56 | 3.45 | 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 | 8.32 | 1.57 | β | 2122 | -0.251 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.190* | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 2043* | β | β |
| Cavallo et al. | 2024 | 7.14 | 2.29 | β | 1905 | -0.810 | β | β | β |
| Hunt & Reffert | 2023 | 8.70 | 1.76 | 1.32 | 1211 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 1109 | β | 33 | β | β |
| Cantat-Gaudin et al. | 2020 | 8.79 | 1.07 | β | 1905 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 10.65 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 10.65 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 1.22 | 0.64 | β | 1109 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.22 | 0.64 | β | 1109 | β | β | β | β |
| Dias et al. | 2002 | 1.49 | 0.84 | β | 398 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.