VDBH 75
(van den Bergh-Hagen 75; BH 75; vdBergh-Hagen 75; MWSC 1691)
0.31
UTI
0.27
CN
0.18
Cdens
0.38
CC3
0.35
Clit
1.0
Cdup
Nm (P>50%)
27
Core radius and density
1.4 [pc], 0.9 [pc-2]
- CN 0.27 Poorly populated
- Cdens 0.18 Very loose
- CC3 0.38 Low quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
VDBH 75 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below 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 and mass parameters (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 143.824 | -54.632 | 0.398 | -6.287 | 4.12 | 4.667 |
| Hunt & Reffert | 2024 | 143.801 | -54.627 | 0.388 | -6.218 | 4.118 | 38.888 |
| Cavallo et al. | 2024 | 144.237 | -54.594 | 0.399 | â | â | â |
| Hunt & Reffert | 2023 | 143.801 | -54.627 | 0.388 | -6.218 | 4.118 | 38.888 |
| Just et al. | 2023 | 143.673 | -54.697 | â | â | â | â |
| Sampedro et al. | 2017 | 143.7 | -54.7 | â | -1.97 | 1.32 | â |
| Kharchenko et al. | 2016 | 143.673 | -54.697 | â | â | â | â |
| Dias et al. | 2014 | 143.7 | -54.7 | â | -1.37 | 1.83 | â |
| Kharchenko et al. | 2013 | 143.679 | -54.7 | â | -7.31 | 8.06 | â |
| Bukowiecki et al. | 2011 | 143.688 | -54.688 | â | â | â | â |
| Dias et al. | 2002 | 143.7 | -54.7 | â | -1.37 | 1.83 | â |
| Lynga | 1987 | 143.705 | -54.726 | â | â | â | â |
| van den Bergh & Hagen | 1975 | 143.3 | -54.5 | â | â | â | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 2.5 | 1.64 | 2.52 | 236 | 0.380 | 277 | â | â |
| Hunt & Reffert | 2024 | 2.23 | 1.61 | 2.52 | 95 | â | 277(1) | â | â |
| Cavallo et al. | 2024 | 2.24 | 1.54 | â | 295 | 0.380 | â | â | â |
| Hunt & Reffert | 2023 | 2.23 | 1.61 | 2.52 | 95 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 708 | â | 1879 | â | â |
| Kharchenko et al. | 2016 | 5.98 | 3.09 | â | 708 | â | â | â | â |
| Kharchenko et al. | 2013 | 5.98 | 3.09 | â | 708 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 258 | â | â |
| Bukowiecki et al. | 2011 | 2.51(1) | 1.64 | â | 178 | â | â | â | â |
| Dias et al. | 2002 | 2.50 | 1.70 | â | 178 | â | â | â | â |
(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 class: 0.94 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.94 (50th percentile).