VDBH 118
(van den Bergh-Hagen 118; BH 118; vdBergh-Hagen 118; MWSC 1939; ESO 129 20)
0.81
UTI
0.8
CN
1.0
Cdens
0.75
CC3
0.74
Clit
1.0
Cdup
Nm (P>50%)
231
Core radius and density
1.9 [pc], 6.9 [pc-2]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.74 Moderately 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 and mass parameters (see Parameters). It is moderately studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 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 |
| Jadhav & Subramaniam | 2021 | 170.765 | -58.549 | 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 |
| Dias et al. | 2018 | β | β | β | -7.78 | 1.39 | β |
| Dib et al. | 2018 | 170.625 | -58.53 | β | β | β | β |
| Sampedro et al. | 2017 | 170.762 | -58.55 | β | -5.45 | -4.17 | β |
| Joshi et al. | 2016 | 170.625 | -58.53 | β | β | β | 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 |
| Bukowiecki et al. | 2011 | 170.879 | -58.52 | β | β | β | β |
| Dias et al. | 2002 | 170.762 | -58.55 | β | -7.56 | 3.45 | β |
| Lynga | 1987 | 170.718 | -58.546 | β | β | β | β |
| van den Bergh & Hagen | 1975 | 170.15 | -58.267 | β | β | β | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 7.14 | 1.07 | 1.32 | 1160 | -0.251 | 1268 | β | 1 |
| Li et al. | 2025 | 8.32 | 1.57 | β | 2122 | -0.251 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.190(5) | β | β | β |
| Hunt & Reffert | 2024 | 8.70 | 1.76 | 1.32 | 1211 | β | 2043(1) | 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 |
| Jadhav & Subramaniam | 2021 | 8.79 | 1.07 | β | 1905 | β | 3466 | β | 1(1) |
| Cantat-Gaudin et al. | 2020 | 8.79 | 1.07 | β | 1905 | β | β | β | β |
| Kounkel et al. | 2020 | 6.40 | 1.52 | β | 1288 | 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 |
| Dib et al. | 2018 | 1.22 | β | β | 1109 | β | β | β | β |
| Joshi et al. | 2016 | 1.22 | 0.66 | β | 1109 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.22 | 0.66 | β | 1109 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.22 | 0.66 | β | 1109 | β | β | β | β |
| Bukowiecki et al. | 2012 | β | β | β | β | β | 493 | β | β |
| Bukowiecki et al. | 2011 | 1.50(1) | 0.82 | β | 398 | β | β | β | β |
| Dias et al. | 2002 | 1.49 | 0.85 | β | 398 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 0.76 (50th percentile), false positive? (human-assigned).
Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 0.76 (50th percentile), false positive? (human-assigned).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.2696, e_all=0.1917.