VDBH 85
(van den Bergh-Hagen 85; BH 85; vdBergh-Hagen 85; MWSC 1748; ESO 213 05)
0.80
UTI
0.81
CN
1.0
Cdens
0.75
CC3
0.71
Clit
1.0
Cdup
Nm (P>50%)
256
Core radius and density
1.9 [pc], 5.8 [pc-2]
- CN 0.81 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.71 Moderately studied
- Cdup 1.0 Unique
Overview
VDBH 85 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, well 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 mass parameters (see Parameters). It is moderately studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 150.467 | -49.564 | 0.138 | -5.681 | 4.665 | 61.462 |
| Li et al. | 2025 | 150.469 | -49.564 | 0.106 | -5.689 | 4.676 | β |
| Hu & Soubiran | 2025 | 150.476 | -49.568 | β | β | β | β |
| Almeida et al. | 2025 | 150.466 | -49.568 | β | β | β | β |
| Hunt & Reffert | 2024 | 150.466 | -49.562 | 0.142 | -5.659 | 4.652 | 61.253 |
| Cavallo et al. | 2024 | 150.476 | -49.568 | 0.136 | β | β | β |
| Hunt & Reffert | 2023 | 150.466 | -49.562 | 0.142 | -5.659 | 4.652 | 61.253 |
| Just et al. | 2023 | 150.459 | -49.581 | β | β | β | β |
| Jadhav & Subramaniam | 2021 | 150.469 | -49.564 | β | β | β | β |
| Dias et al. | 2021 | 150.466 | -49.568 | 0.101 | -5.704 | 4.656 | β |
| Cantat-Gaudin et al. | 2020 | 150.469 | -49.564 | 0.106 | -5.689 | 4.676 | β |
| SΓ‘nchez et al. | 2020 | 150.467 | -49.567 | β | -5.718 | 4.637 | β |
| Cantat-Gaudin & Anders | 2020 | 150.469 | -49.564 | 0.106 | -5.689 | 4.676 | β |
| Soubiran et al. | 2018 | 150.469 | -49.564 | β | β | β | 60.84 |
| Bica et al. | 2019 | 150.458 | -49.567 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 150.469 | -49.564 | 0.106 | -5.689 | 4.676 | β |
| Sampedro et al. | 2017 | 150.467 | -49.567 | β | β | β | β |
| Kharchenko et al. | 2016 | 150.459 | -49.581 | β | β | β | β |
| Dias et al. | 2014 | 150.467 | -49.567 | β | -5.04 | 7.73 | β |
| Kharchenko et al. | 2013 | 150.465 | -49.585 | β | -3.86 | 8.55 | β |
| Bukowiecki et al. | 2011 | 150.467 | -49.557 | β | β | β | β |
| Dias et al. | 2002 | 150.467 | -49.567 | β | -4.2 | 7.57 | β |
| Lynga | 1987 | 150.485 | -49.643 | β | β | β | β |
| van den Bergh & Hagen | 1975 | 150.0 | -49.4 | 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 | 6.04 | 1.22 | 1.56 | 1441 | -0.157 | 1952 | β | 3 |
| Li et al. | 2025 | 5.95 | 1.65 | β | 1482 | -0.154 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.160(5) | β | β | β |
| Almeida et al. | 2025 | 5.94 | 1.22 | β | 3221 | β | 1853 | β | β |
| Hunt & Reffert | 2024 | 6.13 | 1.61 | 1.56 | 1399 | β | 2050(1) | β | β |
| Cavallo et al. | 2024 | 3.52 | 1.67 | β | 3162 | -0.310 | β | β | β |
| Hunt & Reffert | 2023 | 6.13 | 1.61 | 1.56 | 1400 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 631 | β | 986 | β | β |
| Jadhav & Subramaniam | 2021 | 7.48 | 1.10 | β | 2291 | β | 3984 | β | 3(1) |
| Dias et al. | 2021 | 5.94 | 1.22 | β | 3221 | -0.028 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 7.48 | 1.10 | β | 2291 | β | β | β | β |
| Kounkel et al. | 2020 | 4.81 | 1.16 | β | 1862 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 7.41 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 7.41 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 7.41 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 2.79 | 2.63 | β | 631 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.79 | 2.63 | β | 631 | β | β | β | β |
| Bukowiecki et al. | 2011 | 15.05(1) | 0.69 | β | 708 | β | β | β | β |
| Dias et al. | 2002 | 1.50 | 0.73 | β | 708 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.23 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.23 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.0634, e_all=0.1542.